The galaxy presents as a relatively smooth, elliptical-like system. There is a bright, concentrated central bulge that appears nearly spherical. The color of this central region is noticeably redder compared to the outer regions of the galaxy. The outer disk/halo appears significantly fainter than the core, with a bluer hue. No obvious spiral arms or dust lanes are visible. The overall shape is very round. There are no signs of major mergers or tidal disturbances. The faint outer regions suggest a gradual decline in stellar density with radial distance from the nucleus. The galaxy appears to be relatively isolated, with no nearby companions visibly interacting.
