The galaxy presents a relatively smooth and elliptical morphology. It exhibits a concentrated central bulge region that appears yellowish-white, possibly indicating an older stellar population dominating the core. Moving outward from the center, a faint, diffuse halo of light surrounds the main body. There are subtle color variations observed in the galaxy, with a slight bluish tint noted in the outer regions. These hints of bluer colors possibly suggesting the presence of some younger stars and ongoing, albeit low level, star formation within the disk. Overall, the galaxy appears undisturbed, with no obvious signs of recent mergers or tidal interactions and a round shape.
