The galaxy appears to be relatively compact and smooth in overall structure. It has a generally rounded morphology. There is no prominent disk or spiral arm structure that is readily apparent. The galaxy displays a significant central bulge that appears to be elliptical in shape.

The color gradient across the galaxy suggests varying stellar populations or dust content. The central region exhibits a reddish-yellow hue, possibly indicative of older, cooler stars or dust obscuration. Progressing outwards from the center, the colors shift towards a slightly bluer tone, indicating the presence of a younger stellar population in the galaxy's outer regions.

There is a slight asymmetry in the morphology, hinting at possible tidal interactions or minor disturbances. There is no obvious major merger or strong tidal tails present, though some faint features suggest the possibility of ongoing interactions or recent minor mergers.
