The galaxy appears as a centrally concentrated object with a smooth overall structure. The core region exhibits the brightest luminosity. The shape is more in between of round and elliptical than clearly circular or elongated. Hints of non-uniform light distribution and subtle disturbances around the central region are observed. There might be some evidence of subtle disk-like features, but the galaxy is primarily smooth in appearance. The color gradient suggests ongoing star formation, albeit not vigorously. The galaxy does not appear to be undergoing a major merger event, although minor disturbances could be occurring.
