The galaxy exhibits a generally elliptical morphology. It appears elongated, approximately three times longer than it is wide, and has a smooth, diffuse light distribution, with no apparent spiral arm structure or significant dust lanes visible. The color is predominantly yellow-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. There are slight indications of a central bulge. No tidal features or signs of major mergers are readily apparent, although subtle asymmetries or minor disturbances cannot be ruled out at this resolution. Overall, it appears to be a relatively evolved, quiescent galaxy.
