The galaxy presents as a diffuse, centrally concentrated structure. It is primarily elliptical in shape, exhibiting a smooth light distribution. The core region appears brighter, fading gradually towards the outer edges. There is a very slight flattening of the galaxy, suggesting it may be closer to an E4 or E5 on the Hubble scale. The galaxy appears to be relatively isolated with no obvious signs of recent major mergers or tidal disturbances. There are hints of a minor asymmetry. The overall color is yellowish. Based on the observed morphology, the galaxy is likely an early-type galaxy dominated by an older stellar population.
