The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a higher surface brightness, appearing more luminous with a subtle reddish-yellow hue. The isophotes appear elongated, suggesting a moderate ellipticity. No distinct spiral arm structures or prominent dust lanes are visible. The outer regions of the galaxy gradually fade into the background, indicative of a diffuse stellar halo. There are no visually apparent signs of major mergers or significant tidal disturbances.
