The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. Fainter, bluer colors are observed extending away from the center. There is no obvious spiral structure or evidence of active star formation regions. The galaxy appears relatively isolated, with no clear signs of ongoing or recent major mergers or tidal disturbances based on the image. The galaxy displays a generally rounded morphology.
