The galaxy presents as a diffuse, elliptical structure with a dominant central bulge. Color gradients suggest an aging stellar population, with a reddish-yellow hue concentrated in the core region, indicating the presence of older, cooler stars. The outer regions appear slightly bluer, possibly indicative of some residual star formation, but overall the galaxy presents a smooth, relatively featureless appearance. There is no indication of spiral arms or a well-defined disk. The morphology is generally smooth, suggesting that the galaxy is relatively undisturbed, possibly due to its isolation. The light distribution is moderately concentrated, and the overall shape is close to round, but with a slight elongation.
