The galaxy presents as a moderately bright, ellipsoidal structure, exhibiting a smooth, featureless morphology. The galaxy's color profile indicates a dominant population of older stars, evidenced by the reddish-yellow hue in the central region, suggesting minimal ongoing star formation. A slight color gradient is visible, transitioning to a bluer tint toward the outer edges, possibly indicating a younger stellar population in the galactic periphery. The object appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions, although a minor disturbance cannot be ruled out. Overall, the galaxy seems to be a passively evolving system with a substantial stellar mass, located at a considerable distance.
