The galaxy presents as a concentrated, elliptical morphology with a smooth light profile, indicating an older stellar population. The central bulge is bright and yellow-white, suggesting a high density of evolved stars. The outer regions exhibit a slightly more diffuse and reddish hue, possibly due to dust or a population of cooler, redder stars. There is no visible evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no obvious signs of recent mergers or major interactions. The overall color indices suggest that star formation activity is low.
