The galaxy appears as a largely featureless elliptical or lenticular system. There is a centrally concentrated, bright bulge region. This core fades gradually into an extended, fainter halo. The overall color suggests an older stellar population, with a yellowish-white hue dominating the central region. The outer regions appear slightly bluer. There is no noticeable dust lane, spiral arm structure, or other significant morphological features. The galaxy exhibits a smooth, rounded shape with no apparent signs of major disturbances or ongoing merger activity. It appears to be a relatively isolated system.
