The galaxy presents a smooth, elliptical morphology, with a concentrated central bulge that exhibits a yellowish hue, potentially indicating an older stellar population within. The outer regions show a gradual decrease in luminosity, extending into a fainter halo. There are hints of bluer colors in the disk possibly indicating areas of ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. The galaxy's shape is close to circular, suggesting that it's being viewed close to face-on.
