The galaxy presents as a relatively smooth, centrally concentrated object. The light profile exhibits a gradual decrease in intensity moving outward from the core, which is suggestive of an elliptical morphology or a spiral galaxy viewed face-on with minimal discernible spiral arm structure. There is a slight color gradient, with the central region appearing more yellow/white, implying a population of older stars. The outer regions appear redder, potentially due to either a population of older, redder stars or dust obscuration. No significant tidal features, dust lanes, or other morphological disturbances are readily apparent, and the overall structure seems relatively undisturbed. The high level of smoothness suggests minimal on-going star formation. The roundness indicates that it is not a disk galaxy that we are viewing edge on. Overall, the galaxy appears to be an evolved system with a large population of relatively old stars and a low rate of star formation.
