The galaxy appears as a relatively compact, smooth object, possibly elliptical in nature. It exhibits a moderate degree of ellipticity, tending towards a somewhat elongated shape. There is no evidence of spiral arms or a prominent disk structure. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness towards its outer edges. The color appears to be dominated by intermediate wavelengths, perhaps due to the presence of an older stellar population. There are no indications of major ongoing mergers or significant tidal disturbances, suggesting a relatively quiescent evolutionary state, with potentially low specific star formation.
