The galaxy presents an overall smooth morphology, suggesting characteristics of an early-type galaxy such as an elliptical or lenticular. There is a bright central bulge with a concentrated light profile, surrounded by a more diffuse, elongated halo. Hints of a possible disk structure are present, though not sharply defined. The galaxy's color appears generally redder, indicative of an older stellar population and lower star formation rate, with perhaps a small amount of more recent activity. Some minor disturbances are present, but the galaxy does not appear to be undergoing a major merging event.
