The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, the light gradually fades into a reddish-brown halo, possibly indicating a lower density of stars or the presence of dust absorption. No distinct spiral arms or disk-like features are discernible. The overall morphology appears smooth and relatively undisturbed, with no obvious signs of ongoing major merger activity. It's round appearance indicates it may be close to face-on. 
