The galaxy presents a largely smooth, elliptical morphology with a concentration of light towards the center, suggesting a significant bulge component. It exhibits a color gradient, transitioning from a warmer, yellower hue in the central regions to a slightly cooler tone toward the outskirts. There is little indication of spiral arms or significant dust lanes. The round shape suggests it is likely an elliptical galaxy, with no major mergers or disturbances. The overall color profile indicates a population of older stars, suggesting relatively low current star formation.
