The galaxy presents as a coalescing system, possibly undergoing a merging process. It exhibits a disturbed morphology, with evidence of tidal features or faint plumes extending from the primary galactic body. The galaxy appears to be composed of at least two distinct nuclei or regions of concentrated luminosity, suggesting interaction or close proximity between separate galaxies. The overall color is indicative of an older stellar population with ongoing star formation. The galaxy exhibits an elliptical appearance with a smooth light distribution across its disk.
