The galaxy presents as a relatively smooth, elliptical-like structure with a somewhat elongated shape. A central bulge is visible, exhibiting a concentrated, bright intensity. The surrounding halo appears more diffuse, with a gradual decrease in luminosity extending outwards. There seems to be some sort of interaction occurring between the central area and a smaller concentration of material just outside the main part of the galaxy. The color profile indicates a slightly redder hue in the central regions, transitioning to bluer tones in the outer disk, suggesting varying stellar populations or dust content across the galaxy.
