The galaxy presents as a moderately luminous, elliptical-like structure. Its core is a bright, concentrated region, suggesting a high density of stars. The overall color appears reddish-yellow, possibly indicating an older stellar population with a lower proportion of young, hot stars. The galaxy exhibits a smooth, diffuse profile, with no discernible spiral arms or distinct features indicative of active star formation regions. There is a slight asymmetry to the galaxy, though it does not appear to be undergoing a major merging event. The overall morphology suggests a relatively relaxed system that may have undergone significant evolution.
