The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There is little evidence of spiral arm structure or significant dust lanes. The light profile appears largely spheroidal, with a gradual decrease in luminosity from the core outwards. The color appears generally redder, suggestive of an older stellar population, although some bluer hues are present. The overall structure does not indicate any major ongoing mergers or tidal disturbances, and the galaxy appears relatively undisturbed. 
