The galaxy appears to be a relatively compact object. Its overall morphology is smooth with a generally elliptical shape. There is a subtle hint of a disk-like structure present, potentially with a minor disturbance. The light profile suggests a concentration of stellar mass in the central region. Its red color indicates an older stellar population. The galaxy does not show any obvious signs of recent major merger activity, but there may be minor tidal features or asymmetries suggesting a past interaction or ongoing minor disturbance. The galaxy exhibits a weak, but measurable, level of on-going star formation.
