The galaxy presents as a single, largely homogenous object with a smooth morphology. It appears elliptical in shape, close to circular, with no discernible spiral arms or distinct features. There is a noticeable concentration of light toward the center, which fades gradually toward the outer edges. The color is a soft yellow-white in the core, shifting toward a slightly bluer hue in the outer regions. There is no indication of ongoing major merger activity or significant tidal disturbances, although minor irregularities cannot be ruled out given the resolution. Based on the color and morphology, it is likely a galaxy composed primarily of older stars, with a relatively low rate of star formation.
