The galaxy presents as a relatively compact, elliptical-like structure. The light distribution appears centrally concentrated, with a smooth, diffuse profile fading outward. There are no clear spiral arms or a distinct galactic disk visible. The galaxy's color appears somewhat reddish-orange, suggestive of an older stellar population, and potentially minimal recent star formation. There might be some minor disturbances but the galaxy overall appears to be isolated and undisturbed. The roundness of the galaxy could be described as mostly round.