The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated bulge that is notably luminous with a yellow-orange hue. The outer regions show a gradual decrease in surface brightness, fading into the background. A faint, diffuse halo surrounds the central region. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears to be isolated, with no clear signs of ongoing major mergers or tidal disturbances.
