The galaxy presents a centrally concentrated, elliptical morphology. The core exhibits a bright, relatively uniform luminosity profile, suggesting a high stellar density. The overall color appears relatively red, indicative of an older stellar population. The surface brightness decreases gradually from the core outward, displaying a smooth, diffuse halo. There is no discernible spiral structure or prominent dust lanes. The galaxy appears largely undisturbed, without evidence of recent major mergers or tidal interactions. It has an apparently high Sersic index. There is no evidence of active star formation.
