The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy has a generally round morphology, showing minimal signs of significant disturbances or merging activity. The color gradient suggests an older stellar population, with the central region appearing more yellowish, indicative of a population dominated by evolved stars. There is minimal evidence of dust lanes or spiral arm features. It does not show a notably high rate of star formation. The overall appearance suggests a massive, early-type galaxy.
