The galaxy presents with a generally elliptical morphology. Its central region exhibits a high degree of luminosity, suggestive of a concentrated stellar population, possibly an older population. The isophotes appear somewhat elongated, deviating from a perfectly circular shape. The galaxy's light profile fades gradually from the center outwards, indicating a diffuse stellar halo. There is evidence of some asymmetry within the galaxy's structure, perhaps a sign of minor tidal interactions or recent disturbances. The color appears to be slightly redder towards the center, while the outer regions display a bluer tinge, hinting at differing stellar populations. Overall, it shows properties consistent with a disk galaxy with possible disturbances.
