The 92 ETGs galaxies in this list are presented in Atlas3D Paper XXIX, Duc et al., 2014, MNRAS in press. See tables 2 and 3 for explanations on the morphological class adopted here. Clicking on the galaxy name gives access to the jpeg true color images, surface brightness and color maps, residual images after galaxy model subtraction. Images may be explored with a navigation tool. A pdf version of the image catalog is available here.
| Galaxy | Class | Comments |
| NGC0448 | I+s | The ETG is in a tidal interaction with a disturbed companion. |
| NGC0474 | M+s+r+ph | The ETG is surrounded by multiple concentric shells and hosts several radial streams. Its outer halo reaches the disk of the unperturbed companion spiral galaxy, NGC 0470. |
| NGC0502 | M+t?+r?+ah-wc-h | The stellar halo of the ETG is asymmetric, possibly due to the presence of a diffuse tidal tail and/or a shell. |
| NGC0509 | R-pc | |
| NGC0516 | R-pc | |
| NGC0524 | U-pc-h | The ETG is surrounded by galactic cirrus and extended halos from bright stars, preventing the detection of fine structures around it. |
| NGC0525 | R-pc-h | |
| NGC0661 | U+ah-pc | The ETG is surrounded by galactic cirrus and extended halos from bright stars, preventing the detection of fine structures around it. |
| NGC0680 | I+t+s+r+ph+wl-wc | The ETG is tidally disturbed, showing two extended tidal tails, and an asymmetric stellar halo. It has a bright edge-on companion in its vicinity. Whether the tidal tails result from this on-going interaction or a past major merger is unclear. |
| NGC0770 | I+t-pc | The ETG lies within a prominent tidal tail. It is likely a satellite of the massive perturbed spiral NGC 0772, and is currently tidally disrupted. |
| NGC0936 | C+s+wl | A stellar stream hosting a tidally disrupted companion wraps around the ETG. |
| NGC1023 | U+ah-h | The stellar halo of the ETG seems to be slightly disturbed, but the extended halos of two bright nearby stars hamper the classification. |
| NGC1121 | U-h | The ETG totally lies within the reflection halo of a bright star, preventing the detection of fine structures. |
| NGC1222 | M+t+r?+ph+pl | The ETG exhibits multiple signs of a relatively recent gas-rich merger: tidal tails, perturbed main body, dust lanes. |
| NGC1248 | R-pc-h | The ETG does not show any evident sign of disturbances although it makes a close pair with the undisturbed spiral galaxy Mrk 604. |
| NGC1266 | C+s?+wl-pc | The ETG has several low mass companions, with possibly a tidally disrupted one. Note however the high level of cirrus contamination. |
| NGC1289 | U+s?+wl-pc | Model subtraction of the ETG reveals a slightly perturbed central body with possibly a faint stream. However Galactic cirrus prevents a firm classification. |
| NGC1665 | U-h | The ETG is surrounded by a ring like structure probably made of old stars. Prominent Galactic cirrus is present in the field. |
| PGC016060 | C+d+pl | The galaxy is surrounded by a warped star-forming ring, and is possibly interacting with an early-type companion to the East. |
| UGC03960 | R-h | The ETG is apparently relaxed though the halo of a nearby star hampers the detection of faint tidal streams. |
| NGC2481 | I+t?-wc | The ETG and its disturbed companion NGC 2480 make an interacting pair. The prominent tidal tails shown by the system likely come from the companion galaxy. |
| NGC2577 | C+s-wc | The ETG has a regular main body with one radial stellar stream sticking out to the North, hosting a possible progenitor. |
| NGC2592 | C+s+r-pc | The ETG is surrounded by cirrus. However the filament to the East is most likely a stellar stream as it hosts a putative progenitor. |
| NGC2594 | U+wl-pc-h | Galaxy classification is hampered by the presence of a nearby bright star and cirrus. The long filament to the South is most likely a cirrus. |
| NGC2695 | R | |
| NGC2685 | M+t?+ph+d+pl | The ETG exhibits a prominent perturbed star-forming disk and dust lanes, indicative of a rather recent gas-rich merger. |
| NGC2698 | I+t+ah-h | The ETG is involved in a tidal interaction with another ETG, NGC 2699. A diffuse bridge links the two galaxies. Besides, a large diffuse tail or stream wraps around the galaxy. |
| NGC2699 | I+t+s+r+ph | The ETG is involved in a tidal interaction with another ETG, NGC 2698. A diffuse bridge links the two galaxies. The main body is highly perturbed with multiple tails and streams around it. |
| NGC2764 | M+t+r+ph+pl-h | The ETG exhibits multiple tidal tails, shells and dust lanes, indicative of a relatively recent major wet merger. |
| NGC2768 | C+s?+r?+ah-h | The main body of the ETG is pretty relaxed, though asymmetric, and exhibits to the South either a stellar stream or shells, telling about a past merger. |
| NGC2778 | R | The ETG does not show any evidence of a tidal perturbation though it makes a close pair with the massive companion NGC 2779. |
| PGC028887 | U-h | The ETG is apparently relaxed, though its stellar halo hosts two possible companions, one with a stream (but the physical association is unsure). The presence of an extended reflection halo is problematic for the galaxy classification. |
| NGC3073 | I+t?+ah | The ETG may be a satellite of the nearby massive edge-on spiral NGC 3079. It exhibits an asymmetric main stellar body. Model subtraction reveals a possible diffuse tidal tail. |
| UGC05408 | C+s+wl-h | Two streams wrap around the ETG, revealing one or two minor mergers. |
| NGC3193 | I-h | The ETG makes an interacting pair with the tidally perturbed galaxy NGC 3189. It is embedded in the reflection halo of a bright star, preventing the detection of tidal tails. |
| NGC3226 | I+t?+s?+r?+ph+wl | The ETG is in close tidal interaction with the strongly disturbed spiral galaxy NGC 3227. The system is surrounded with multiple tidal tails. |
| NGC3230 | R-wc-h | |
| NGC3245 | I+r | Multiple shells are revealed by the ETG model subtraction. The galaxy is likely in tidal interaction with the edge-on, slightly warped, spiral, UGC 5662. |
| NGC3379 | R+r? | The ETG has a regular main body. The model subtraction possibly reveals shells. The galaxy makes a pair with the ETG NGC 3384. |
| NGC3384 | I+ah | The main stellar body of the ETG is asymmetric. It makes a pair with the ETG NGC 3379 and is believed to have been involved in a fast encounter with M96 that possibly formed the huge HI ring surrounding the system (known as the Leo Ring). |
| NGC3400 | R | |
| NGC3414 | I+s+ph | The disturbed ETG is in interaction with the tidally disturbed companion NGC 3418. It is crossed by a very extended South-North stellar stream. Its progenitor is visible to the South. To the North, the stream ends in a shell-like structure. |
| NGC3457 | R+wl-wc | |
| NGC3489 | R+wl | The roundish red halo around this relaxed ETG is likely caused by an internal reflection of the bright nucleus. |
| NGC3522 | R+s? | A stream hosting a possible progenitor is visible 50 kpc North of this relaxed ETG. Whether it is a disrupted satellite is unclear. |
| NGC3599 | R | |
| NGC3605 | U-h | The ETG is observed towards the halo of its companion NGC 3607. This prevents the detection of fine structures. |
| NGC3607 | I+ah+wl-h | The stellar halo of the ETG is slightly asymmetric. It makes a compact group with the ETGs NGC 3608 and NGC 3605. |
| NGC3608 | I+r?-h | Possible fine structures are visible on the image with the ETG model subtracted. It makes a close physical pair with the ETG NGC 3607. |
| NGC3613 | C+s+r?+ph-h | The subtraction of the ETG model disclosed a prominent stream and several other fainter fine structures. The three objects to the North-East are background galaxies. |
| NGC3619 | M+s+r+ph+pl | The main body of the ETG is strongly perturbed. Multiple shells are visible as well as a stellar stream crossing the galaxy from South to North. |
| NGC4026 | R | The ETG exhibits a strong slightly warped bar. The roundish red halo around the ETG is likely an artefact caused by a reflection of the bright nucleus. |
| NGC4036 | C+s+wl | Remnants of minor mergers are visible around and towards the ETG. It is unclear whether it is weakly interacting with the spiral galaxy NGC 4041, which seems slightly perturbed. |
| NGC4278 | R-h | The companion of the galaxy, the ETG NGC 4283, is located towards its stellar halo, but the two galaxies have a large velocity offset and are likely not interacting. |
| NGC4283 | U-h | The ETG is located towards the stellar halo of the ETG NGC 4278, hampering its classification. The two galaxies have a large velocity offset and are likely not interacting. |
| NGC5173 | C+s?+ah | The ETG, located in a group, is slightly perturbed and exhibits weak signs of minor accretion. |
| NGC5198 | C+s+r | The ETG exhibits a 90 kpc long narrow stellar stream to the West, hosting a disrupted progenitor. |
| NGC5322 | M+r+ah | Several shells are disclosed by the ETG model subtraction. |
| NGC5342 | R+wl | |
| NGC5379 | I+t+ah+wl | The ETG is tidally disturbed by the interaction with the massive spiral NGC 5389. |
| NGC5422 | R+pl-h | The ETG hosts a prominent dusty edge-on disk. |
| NGC5473 | R-h | |
| NGC5481 | R-wc | The ETG is relaxed but makes a close pair with the undisturbed spiral galaxy NGC 5480. |
| NGC5485 | M+t?+s+ph+pl | The stellar body of the ETG is disturbed. It possibly exhibits diffuse tails, streams and prominent dust lanes. |
| PGC050395 | R | |
| NGC5507 | I+t+ah | The ETG is in tidal interaction with the perturbed spiral NGC 5506: its main body is warped. Extended diffuse emission is seen to the South and West. |
| NGC5557 | M+t+r+ph-h | The external regions of the ETG are tidally perturbed. Two long tails emanate from it. The tail to the East hosts confirmed metal-rich tidal dwarf galaxies. |
| NGC5582 | R+d-h | A LSB blue star-forming spiral disk surrounds the relaxed stellar bulge of the ETG. |
| NGC5574 | I+t+ph-h | The ETG is tidally perturbed by the interaction with the ETG NGC 5576. A prominent large tidal tail emanates from it. |
| NGC5576 | I+r+ph | The ETG is strongly perturbed, likely following the tidal interaction with the ETG companion NGC 5574. |
| NGC5631 | M+s+r+ah+wl | The ETG exhibits multiple internal shells, and a curved stream in its outskirts. |
| NGC5638 | C+s | A stream ending with a shell like structure is visible to the South of the ETG. |
| IC1024 | C+s+ph+pl | The ETG shows signs of perturbations and dust lanes. One or two stellar filaments wrap around it. |
| UGC09519 | R+d+pl | The ETG is surrounded by a LSB star-forming disk. It exhibits prominent dust lanes in its central regions. |
| NGC5838 | R-h | |
| NGC5866 | M+ph+wl-h | The stellar body of the ETG is perturbed, but no fine structure is clearly observed. |
| NGC6014 | U+s?+ah+wl-wc | The main body of the ETG exhibits some underlying ring-like substructures, dust lanes and is slightly asymmetric. A filament (stellar or cirrus) of unknown origin is visible to the East. |
| NGC6017 | R+wl | The central bar of the ETG is perpendicular to the main axis of the stellar halo. |
| PGC056772 | R+wl | |
| PGC058114 | R+pl-h | |
| NGC6278 | C+s?-wc | The ETG makes a close pair with the unperturbed spiral NGC 6276. A possible stream is seen to the North, and fainter ones are disclosed by the model subtraction. |
| NGC6547 | R-h | The morphological classification is hampered by the presence of numerous foreground stars. |
| NGC6548 | R-wc | |
| NGC6703 | U+wl-pc-h | The ETG is located within a galactic cirrus and cannot be classified. |
| NGC6798 | U-pc-h | The ETG is surrounded by multiple filamentary cirrus-like structures. |
| NGC7280 | C+s | The ETG makes a pair with star-forming companion UGCA 429. Two faint streams are visible to the South. |
| NGC7332 | I+ah+d | The disk of the ETG seems slightly warped. It is likely in tidal interaction with the nearby spiral galaxy NGC 7339. |
| NGC7457 | R-pc-h | The filament to the East of the ETG is most likely a cirrus and not a stellar stream. |
| NGC7454 | U-pc-h | The presence of multiple narrow filaments due to cirrus prevents any classification. |
| NGC7465 | I+t+ph+d+pl-wc-h | The ETG hosts a tidally perturbed star-forming disk. It is interacting with the irregular galaxy NGC 7464 and possibly the spiral NGC 7463. |
| NGC7693 | R-wc | The ETG is relaxed though it makes a close pair with an undisturbed spiral to the South of unknown redshift. |
| NGC7710 | R+pl-wc | The ETG has a remarkable thin dusty edge-on disk. |