The galaxy presents a largely smooth, centrally concentrated morphology. It appears generally elliptical in shape, showing a diffuse, extended halo that gradually fades into the background. The core region is significantly brighter than the outer regions and exhibits a slightly bluer hue, implying a potentially younger stellar population or enhanced star formation in that area. The overall color of the galaxy trends toward redder hues in the outer regions, possibly indicative of an older stellar population dominating these areas. There is a slight indication of minor disturbance within the galaxy's structure, but overall it is not heavily disrupted.
