The galaxy presents as a somewhat smooth, centrally concentrated object. There is a bright, unresolved core suggestive of a possible active galactic nucleus or a dense stellar population. Fainter, diffuse light extends outwards from the central region, displaying hints of a disk-like structure. Subtle color variations are apparent, with a bluer hue around the main body. The color suggests ongoing star formation. Some irregular features are present, possibly indicative of minor disturbances or ongoing interaction. The galaxy does not appear to be undergoing a major merger, though some interaction cannot be ruled out.
