The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a largely elliptical morphology with hints of a flattened disk. The color is dominated by light in the green and red bands, with a noticeable contribution from the blue band. There are no prominent spiral arms or significant dust lanes visible. The galaxy displays a relatively smooth light profile, with no large-scale disturbances or tidal features immediately apparent, though there are some minor distortions in the outer regions which may be indicative of an ongoing or past minor merger event. It is classified as a lenticular or early-type spiral galaxy, and it does not seem to be actively undergoing significant star formation. The core shows a bright, concentrated region, possibly indicating the presence of an older stellar population and potentially a supermassive black hole at its center.
