The galaxy appears as a centrally concentrated, elliptical or lenticular-shaped object. Its overall color profile suggests a population of older stars, with a noticeable yellowish-orange hue dominating the galaxy's central region, transitioning to slightly bluer tones in its outer regions. The light is generally smooth and diffuse, with no distinct spiral arm structures or prominent dust lanes visible. There are no obvious signs of ongoing major mergers or tidal disturbances. The galaxy's form can be described as being largely in between a perfect sphere and elongated shape. There is a high likelihood that the galaxy is relatively undisturbed with no ongoing mergers.
