The galaxy presents as a largely smooth, elliptical-like structure. The core region appears as a bright, concentrated area. The light profile suggests minimal discernible spiral arm features or significant dust lane obscuration. The color gradient transitions from a yellowish core to a redder halo, which may indicate an aging stellar population. There is no obvious evidence of a major merger event. The morphology appears relatively undisturbed, showing perhaps very minor disturbances in the surrounding region. The structure appears nearly round.
