The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It exhibits a roughly elliptical shape with a high degree of roundness. There is no visible evidence of spiral arms, bars, or significant disk structure. The core region displays a bright, yellowish-white luminosity, possibly indicative of an older stellar population. The outer regions of the galaxy gradually fade into the background sky, displaying a slightly reddish hue. There are no apparent tidal features, dust lanes, or signs of ongoing merger activity. The galaxy appears to be relatively undisturbed.
