The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The overall color is yellowish-white, suggestive of an older stellar population. The light distribution is centrally concentrated, fading gradually towards the outer edges. The shape is close to round, though with a possible slight elongation. No signs of major ongoing mergers are immediately apparent, though there may be minor disturbances present. The galaxy is estimated to be a significant size with a substantial stellar mass, and low star formation rate.
