The galaxy presents a predominantly smooth morphology, appearing largely elliptical in shape. It exhibits a concentrated central bulge that fades into a less structured halo. Color gradients suggest a relatively older stellar population, particularly within the central region, with a shift toward redder hues. There is an absence of clearly defined spiral arms or significant dust lanes. Faint features are present on its periphery that may indicate recent star formation, or could be tidal debris from a minor merger event. No indications of a clear active galactic nucleus are apparent in this view, with the galaxy appearing relatively quiescent.
