The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge that is bright, with a gradual decrease in luminosity moving outward. The overall shape appears somewhat flattened, transitioning from a rounder center to a more elongated outer region. The galaxy's color profile suggests a population of older stars. There is minimal evidence of active star formation regions or distinct spiral arms, indicating a more quiescent state. The general morphology suggests that the galaxy is unlikely to be undergoing any major merger events. The light distribution is primarily uniform across the galaxy's surface.
