The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. There is a chain of three relatively bright, compact regions along a curved axis, all with an overall reddish-orange hue. These could be individual galactic nuclei or areas of intense star formation triggered by tidal interactions. A faint tail-like structure extends from one of the central bright regions, indicating possible tidal disruption. The system appears to be relatively luminous, with a non-negligible star formation rate. The system's overall shape deviates significantly from a typical elliptical or spiral structure. It looks to be experiencing gravitational disturbance.
