The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a notable lack of distinct spiral arm structures or significant dust lanes. The galaxy’s color profile suggests a population of older stars, with a redder hue dominating the central bulge and inner regions. The outskirts of the galaxy appear slightly bluer, potentially indicating some ongoing, albeit subdued, star formation activity. Overall, the galaxy appears relatively undisturbed, without significant signs of recent mergers or tidal interactions. It possesses a round shape. There is likely low-level star formation. The object exhibits a substantial mass, indicative of a mature system.
