The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. The light profile appears to be dominated by an older stellar population, exhibiting a yellowish-red hue, particularly concentrated toward the galactic center. There is little evidence of spiral arm structure or distinct dust lanes. Subtle color gradients suggest the presence of some regions with ongoing, though likely limited, star formation. The overall structure points towards a system with a dominant spheroidal component, possibly an elliptical galaxy or a lenticular galaxy seen at a significant inclination. There is no immediately apparent evidence of strong tidal interactions or a recent major merger event. The galaxy has a moderate redshift.
