The galaxy presents as a centrally concentrated, elliptical-like structure. The central region exhibits a bright, yellowish-white hue, indicating a substantial population of older stars. This core gently diffuses outwards, transitioning to a slightly reddish color in the outer regions. No distinct spiral arms or significant dust lanes are discernible. The overall morphology suggests a galaxy that is relatively smooth and rounded in appearance. There are no apparent signs of ongoing major mergers or tidal disturbances. It exhibits a substantial mass and a very low rate of star formation.
