The galaxy appears to be a relatively smooth, elliptical system. Its morphology is dominated by a centrally concentrated bulge that fades gradually into the surrounding halo. There is a subtle disk-like component visible, however no clear spiral structure is discernible. The galaxy exhibits a mild elongation, with an apparent axis ratio suggesting a shape that is somewhat in between round and cigar shaped. There appears to be some minor disturbance in the symmetry of the outer halo, perhaps indicating a past interaction or minor merger event. Overall, the galaxy presents a mature, relatively quiescent system without substantial ongoing star formation. The galaxy appears to be a luminous, massive system. The lack of prominent blue color suggests an older stellar population dominating its emission.