The galaxy presents a generally smooth, elliptical morphology. Its core region appears bright and concentrated, exhibiting a yellowish-white hue. The light profile suggests a centrally dominant stellar population, possibly composed of older stars. A faint, diffuse halo surrounds the core, gradually fading into the background sky. There is no apparent spiral arm structure or prominent dust lanes visible in this image, which further supports its classification as an elliptical galaxy. The overall shape seems relatively undisturbed, with no noticeable tidal features or asymmetries, indicating a low probability of recent major merger events.
