The galaxy presents as a centrally concentrated, elliptical form. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. The outer regions display a gradual fading, indicating a decreasing stellar density with radial distance. There is little to no evidence of spiral arms or significant dust lanes; the morphology appears largely smooth and featureless. Overall, the galaxy appears relatively undisturbed, with no obvious signs of ongoing mergers or major tidal interactions. The shape is approximately in between round and cigar shaped, being elliptical.
