The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears relatively even, indicating a lack of significant spiral arm features or distinct dust lanes. The core exhibits a bright, yellowish-orange hue, likely due to an older stellar population dominating the central regions. The outer regions display a gradual decrease in luminosity. Overall, the galaxy appears to be relatively undisturbed, lacking any obvious signs of major mergers or significant tidal interactions. The shape is not perfectly round but more oval.
