The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge that dominates its overall light profile. The galaxy exhibits a noticeable flattening, suggesting a degree of rotational support. The color gradient indicates a relatively older stellar population, particularly within the central bulge. Faint hints of a surrounding halo or extended stellar distribution are barely discernible around the central body of the galaxy. There is no evidence of spiral arms or significant dust lanes. The overall appearance suggests an early-type galaxy in a relatively quiescent state of star formation.