The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity outward. The color is predominantly yellowish-red, suggesting an older stellar population and relatively low levels of current star formation. No obvious spiral arm structures or significant dust lanes are discernible. The galaxy appears to be isolated, without any clear signs of ongoing major mergers or tidal disturbances, suggesting a relatively undisturbed evolutionary history. A slight elongation in the distribution of light is present, although the overall shape is close to circular.
