The galaxy presents a largely smooth, elliptical morphology. The central region is characterized by a bright, concentrated nucleus exhibiting a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the light intensity gradually decreases, transitioning to a more reddish color. There are no apparent spiral arms or distinct features indicative of ongoing major mergers or significant tidal disturbances. Subtle variations in color and intensity are present, potentially indicating variations in stellar populations or dust distribution within the galaxy. The overall form appears relatively relaxed and symmetric.
