The galaxy presents as a relatively smooth, elliptical-like structure. Its light is concentrated in the center, with a gradual decrease in brightness towards the outer edges. The core region exhibits a yellow-white hue, suggesting an older stellar population. There is a faint, diffuse blue halo surrounding the central bulge, potentially indicating some level of ongoing or recent star formation, although at a low rate. The overall shape appears nearly round but not perfectly circular, tending towards a more flattened elliptical form. No obvious signs of a major merger event are discernible. Subtle irregularities or disturbances might be present, but the overall impression is one of a well-defined, relatively undisturbed galactic morphology.
