The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. It has a bright, compact core that gradually fades into its outer regions, showing a lack of distinct spiral arms or disk-like features. There appears to be some slight asymmetry in the outer halo but overall it looks fairly round in appearance. There are no obvious signs of ongoing major merger activity, such as tidal tails or strong distortions in its overall morphology, though minor disturbances cannot be ruled out. The galaxy exhibits a subtle color gradient, with a slightly bluer hue in the center, suggesting the presence of some ongoing star formation. 
