The galaxy exhibits a generally elliptical morphology, appearing mostly smooth and spheroidal in structure. The light distribution is concentrated towards the center, with a gradual decrease in luminosity outwards. The central region is characterized by a bright, yellowish core, suggesting a population of older stars. The outer regions show a fainter, more diffuse halo of light. There are no obvious signs of strong spiral arms or a distinct disk component. The galaxy appears to be relatively undisturbed, with no clear evidence of ongoing major mergers or tidal interactions. Faint hints of possible minor disturbances can be seen on one side of the galaxy, but the general form is largely unperturbed. The overall color indicates a redder stellar population, typical of elliptical galaxies with low star formation rates.
