The galaxy appears as an elliptical or lenticular type, characterized by a smooth, diffuse morphology. Its overall shape is generally rounded, with minimal evidence of spiral arms or significant disk-like structures. The light distribution appears concentrated toward the center, indicative of a substantial galactic bulge. The color profile suggests a population dominated by older stars, exhibiting a yellowish-orange hue. There are no prominent signs of active star formation regions or significant dust lanes discernible within the observable structure. Slight asymmetrical features may hint at possible past minor interactions, but overall the galaxy seems to be relatively undisturbed. The galaxy's estimated size suggests it is a moderately sized galaxy in terms of spatial extent.
