The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, with a concentration of light toward the galactic center. A distinct color gradient is observed, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy fade into a less defined, somewhat bluer halo. There is no discernible spiral structure or significant dust lane features. The overall appearance suggests a galaxy that has largely ceased active star formation. There is no evidence of any major disturbances or ongoing mergers.
