The galaxy appears to be a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density. The overall color of the galaxy leans toward the redder end of the spectrum, indicating a population of older, cooler stars. There is a subtle asymmetry in the outer regions, hinting at a possible interaction or past merger event. Some faint, blue-ish tinged regions can be seen on the periphery of the galaxy, possibly areas of relatively recent star formation, although not particularly active. The overall shape of the galaxy seems mostly round. There does not appear to be any major ongoing merger activity and there are no obvious spiral arms or distinct features indicating a disk-like structure.
