The galaxy appears as a centrally concentrated, largely featureless elliptical system. It presents with a smooth, rounded morphology, showing no obvious spiral arms or significant disk-like features. The core is bright and diffuse, suggesting a high density of stars in the central region. The color gradient transitions smoothly from a slightly bluer hue in the outer regions to a more reddish-yellow color toward the galactic center. There is no indication of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure. The overall appearance suggests a relatively evolved stellar population with a diminished rate of star formation, consistent with an elliptical morphology.
