The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge with a high degree of symmetry. The outer regions of the galaxy appear fainter, exhibiting a gradual decrease in luminosity from the center outwards. The color appears to be generally yellow-white, possibly indicating an older stellar population with lower rates of star formation. The galaxy does not show any obvious signs of spiral arms or a significant disk structure. There are no clear signs of ongoing major mergers or tidal disturbances, although a slight asymmetry in the outer regions could suggest minor interactions.
