The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue, potentially indicating an older stellar population. There is some indication of a flattened disk-like structure surrounding the central bulge. The outer regions of the galaxy show a decrease in surface brightness, fading into the background. There is a hint of bluer regions in the disk. No signs of major disturbances or ongoing mergers are readily apparent. The overall morphology suggests a galaxy that has largely settled into a stable, relatively quiescent state.
