The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the light intensity decreases gradually, transitioning to a more reddish color profile in the intermediate regions. The outer edges of the galaxy fade smoothly into the background, with no apparent sharp boundaries. The overall structure lacks any distinct features such as spiral arms or dust lanes, reinforcing its classification as an elliptical galaxy. There are no obvious signs of ongoing major mergers or significant tidal disturbances in its morphology.

