The galaxy presents as a relatively smooth object, exhibiting a primarily elliptical morphology. Its shape appears slightly elongated, though not significantly so. The galaxy's color profile suggests a population of older stars, indicated by a reddish hue, but has some hint of some bluer stars as well. There is little evidence of significant spiral arm structure or active star formation regions within the galaxy. The lack of distinct features and its overall smooth appearance implies that this is most likely a relatively evolved galaxy with a large population of older stars. There is no evidence for tidal tails or merging activity, indicating that the galaxy has been undisturbed for a significant period.
