The galaxy presents as a fairly smooth, elliptical structure, characterized by a centrally concentrated luminosity. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The light profile gradually decreases outwards from the center, fading into a more reddish outer halo. The overall shape appears slightly elongated, but not significantly so. There is little to no visible evidence of spiral arms or distinct features usually associated with disk galaxies. No signs of a recent merger event are obvious. The color suggests it is a passive galaxy not undergoing rapid star formation.
