The galaxy presents a morphology consistent with a smooth, elliptical structure. It appears to be a relatively large galaxy, exhibiting a concentrated central bulge that gradually fades into a diffuse halo. A faint disk-like structure appears, though its features are not distinct. The color profile indicates a greater concentration of older stellar populations.

A region with a slightly disturbed shape can be seen at the bottom. This appears to be a region of possible tidal interactions or active star formation. The overall structure suggests a galaxy that is not currently undergoing major mergers.
