The observed galaxy presents a generally elliptical morphology. The central region exhibits high surface brightness, appearing almost uniformly bright and somewhat unresolved in this image. Moving outwards from the core, a fainter, extended disk-like structure is observed, displaying subtle color variations. The galaxy appears predominantly smooth, with hints of a possible minor disturbance or interaction on one edge. Evidence suggests a potential merging event, although the signatures are faint and not definitive.
