The galaxy presents a relatively smooth, elliptical morphology. There is a discernible central bulge, characterized by a concentrated luminosity. The overall color of the galaxy appears to be leaning toward the redder end of the spectrum, implying a population of older stars and reduced current star formation activity. The galaxy appears relatively undisturbed, exhibiting no signs of major mergers or tidal disruptions. It has a high degree of roundness and a lack of distinctive features. Faint and diffuse light extends outwards, with no distinctive arms or spiral structures.
