The galaxy appears to be a relatively smooth, elliptical galaxy. It presents a generally round morphology, with minimal deviation from a circular shape. There is little evidence of spiral arms or significant disk structure. The galaxy exhibits a somewhat concentrated central bulge that is brighter than its surrounding area. The light distribution appears consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy seen at a moderate cosmological distance. There is a slight color gradient visible, with the central region appearing yellower/redder compared to the outer regions. The overall structure suggests a system that has undergone significant dynamical relaxation, with the majority of recent star formation suppressed or absent. No obvious signs of ongoing mergers or tidal disturbances are observed, however this galaxy may have had one in the past, given its proximity to several other galaxies.
