The galaxy appears as a singular, concentrated luminous body. It has a smooth, elliptical morphology with no discernible spiral arm structures or prominent dust lanes. The core of the galaxy exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light gently diffuses outward from the center, transitioning to a reddish color in the outer regions, hinting at an aging stellar population or redshift effects. There is no visual evidence of ongoing major mergers or significant tidal disturbances. The overall form presents as a well-defined, relatively undisturbed elliptical galaxy with a uniform appearance.
