The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. There is little evidence of spiral arms or significant dust lanes. The color gradient suggests a dominant population of older stars, particularly towards the core, which shows a yellowish-orange hue. Moving outward, the galaxy transitions into a bluer shade. The overall shape deviates somewhat from a perfect circle, presenting as slightly elongated. There are no signs of major mergers or significant tidal disturbances in this image. Based on the smooth appearance, older stellar population, and color profile, it is classified as an elliptical galaxy with moderate mass.