The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that graduates smoothly into a more diffuse halo. The color profile indicates a population of older stars, particularly in the central regions, with a yellowish-orange hue dominating the core. The outer regions exhibit a slightly bluer tint, suggesting the presence of younger stellar populations, though to a lesser extent than typically observed in spiral galaxies. There is no discernible dust lane or prominent spiral arm structure. Overall, the galaxy appears well-formed and relatively undisturbed, with no obvious signs of recent major mergers or significant tidal interactions. Its estimated size is approximately 8.6 kpc in radius. The lack of intense star formation implies it is a quiescent galaxy.
