The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated core that suggests the presence of an older stellar population. There is a gradual decrease in luminosity from the center outwards. The axial ratio indicates a shape that is not perfectly spherical, but rather somewhat flattened. The galaxy appears relatively undisturbed, lacking any obvious tidal features or signs of a major merger event. There might be a very faint hint of a disk-like structure, but this is not distinctly pronounced. The overall color profile suggests a galaxy dominated by evolved stars, with a relatively low rate of recent star formation.
