The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The core is yellowish-white, suggesting a population of older stars. The outer regions display a slightly bluer hue, indicating a possible presence of younger stars. The galaxy appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. There are subtle irregularities in the outskirts of the galaxy, possibly indicating minor disturbances. The galaxy is elongated, but not cigar shaped. 
