The galaxy presents as a centrally concentrated system with a smooth, spheroidal morphology. A dominant central bulge is evident, exhibiting a yellow-orange hue, suggestive of an older stellar population. Fainter, bluer extended emission surrounds the bulge, potentially indicative of a disk component with ongoing star formation. The disk appears relatively undisturbed, with no obvious signs of tidal features or strong asymmetries suggesting recent major merger activity. It is slightly elongated, not perfectly circular. Overall, this galaxy appears to be a relatively massive system transitioning towards quiescence, with star formation primarily occurring in its outer regions.
