The galaxy presents as a centrally concentrated, elliptical-like structure. The light profile appears smooth, lacking distinct spiral arm features or a prominent disk. The core region exhibits a pronounced concentration of older stars giving the image a reddish-yellow hue. Moving outward from the core, the galaxy shows a gradual decrease in light intensity, with a transition to a cooler, bluer color. Overall, the morphological structure appears undisturbed, with no apparent signs of tidal interactions or ongoing major mergers.

