The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light profile, with a slight degree of elongation. The central region displays a bright, yellow-white color indicative of an older stellar population. The outer regions fade into a more diffuse halo, exhibiting a subtle redder hue in some sectors. There is some evidence of minor disturbances in the outer edges of the halo, indicating a possible past interaction or accretion event. Star formation appears low within the main body of the galaxy. 
