The galaxy presents an elongated, ellipsoidal morphology. It exhibits a smooth, centrally concentrated luminosity profile, with a bright core that fades gradually toward the outer edges. The central region appears slightly reddish, possibly indicative of an older stellar population. Fainter bluish regions are observed along the edges, perhaps suggesting the presence of younger, hotter stars or ongoing star formation. There is no obvious spiral structure or prominent dust lanes, pointing to a relatively undisturbed system. Based on its apparent shape and color distribution, the galaxy appears to be a lenticular or an elliptical galaxy.
