This galaxy exhibits a generally smooth morphology, indicative of an elliptical or lenticular type. The light profile is centrally concentrated, with a bright core that gradually fades outward. The overall color appears to be relatively red, suggesting an older stellar population with a lower proportion of young, hot stars. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears fairly undisturbed, showing no obvious signs of recent major mergers or tidal interactions. There might be minor disturbances, but the central part is smooth and well-defined.
