The galaxy presents a smooth, elliptical morphology with a slight cigar shape. The central region exhibits a pronounced yellow-white luminosity, indicating a significant population of older stars. Moving outward from the core, the galaxy fades into a diffuse, redder halo, implying a gradual decrease in stellar density and a potential shift toward older stellar populations in the outer regions. There is a subtle disk-like feature extending to the left and right, but it is largely indistinct. Overall, the galaxy appears relatively undisturbed, showing no strong signs of recent major mergers or tidal interactions.
