The galaxy presents as a largely featureless, elliptical or lenticular object. It exhibits a smooth, centrally concentrated light profile with no discernable spiral arm structure or dust lanes. The core region appears bright and somewhat yellowish-orange in color, suggesting a population dominated by older stars. There is a very slight elongation visible. No signs of significant tidal disturbances or ongoing major merger activity are evident. The overall color suggests a low star formation rate. The light distribution indicates a relaxed morphology, implying a relatively quiescent evolutionary state.
