The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears nearly spherical. There is a gradual decrease in luminosity extending outwards from the core, with no apparent spiral arm structure or distinct features like dust lanes or prominent star-forming regions. The galaxy's color profile suggests an older stellar population, as indicated by its reddish-yellow hue. There is no apparent ongoing major merger event, although there is evidence of minor disturbances.