The galaxy appears as a fairly circular, unresolved object. Its light profile exhibits a smooth, centrally concentrated distribution, suggesting a likely classification as an elliptical or S0 galaxy. The color is predominantly yellowish, indicating a relatively old stellar population with minimal ongoing star formation. There is no apparent spiral structure or dust lanes visible. Faint hints of extended light around the core may indicate a diffuse halo or tidal features, but the image resolution limits definitive identification. The overall morphology suggests a system that has largely undergone its major evolutionary processes, with minimal current interaction or significant internal activity.
