The galaxy presents as a centrally concentrated, largely symmetrical structure with a smooth light distribution. There is a high degree of central light concentration. No distinct spiral arms or bar structures are apparent in the image. The galaxy appears nearly circular with no visible dust lanes or prominent features associated with ongoing mergers or tidal interactions. The light profile suggests a spheroidal morphology, possibly an elliptical galaxy or a lenticular galaxy viewed face-on. The color appears generally uniform with a slight suggestion of redder hues, indicative of an older stellar population. The apparent size is relatively compact, and there is no obvious indication of significant star formation activity.
