The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its light profile is centrally concentrated with a gradual decrease in intensity outwards. The overall color is reddish-yellow, suggesting an older stellar population and lower ongoing star formation rate. There's no discernible spiral arm structure or significant dust lane obscuration, and the galaxy exhibits a high degree of rotational symmetry. The morphology indicates a dynamically relaxed system, possibly formed through mergers. The round shape and lack of major disturbances support the classification as an elliptical galaxy that is not currently undergoing a major merging event.
