The galaxy exhibits a morphology suggesting a merger in progress. Its overall shape is somewhat disturbed, showing signs of tidal interactions. A substantial portion of the galaxy's light appears concentrated in a central region, which is elongated and brighter than the surrounding area. There is evidence of a potential tidal tail or bridge extending from this central region, indicating gravitational disruption. The color profile is generally redder, indicative of an older stellar population, though there may be some bluer regions suggestive of ongoing star formation within the merging components. The galaxy is reasonably compact.
