The galaxy appears to be a single, centrally concentrated object. The light is broadly distributed, without well-defined spiral arms or a distinct bar structure. The core of the galaxy exhibits a high surface brightness, with the overall shape being more elliptical than circular. There are some subtle color gradients present. The central region has a yellowish cast that fades to a redder color as you move away from the center. This color gradient may indicate a population shift, perhaps with older, redder stars dominating in the outer regions. There is no obvious evidence of strong tidal features or major ongoing mergers.
