The galaxy presents as a centrally concentrated object with a smooth, somewhat elliptical morphology. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. A gradual color gradient is observed extending outwards from the core, transitioning to a bluish-green halo. This suggests the presence of a younger stellar population and ongoing star formation activity in the outer regions, albeit at a relatively low rate. No significant tidal features or evidence of recent major mergers are apparent, although some minor disturbances cannot be ruled out based on the image alone. The galaxy appears to be a relatively isolated system with no obvious close companions influencing its structure. Its overall appearance aligns with that of an early-type spiral or a lenticular galaxy undergoing a period of moderate star formation.
