The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates outward into a more diffuse halo. The color profile suggests a dominance of older stellar populations, with a yellow-orange hue intensifying towards the core. There is a noticeable lack of distinct spiral arm structures or significant dust lanes. Overall, the galaxy appears relatively undisturbed, with no apparent signs of ongoing major mergers or tidal interactions.
