The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slight ellipticity, appearing more "in between" round and elongated rather than perfectly circular. The light profile suggests a bulge-dominated system, with a gradual decline in surface brightness away from the core. There are a few faint, diffuse extensions that might indicate tidal features or minor disturbances, but no prominent merging or major disruptions are evident. The overall color is consistent with an older stellar population, dominated by redder wavelengths.
