The galaxy appears as a centrally concentrated elliptical galaxy, with a smooth, spheroidal morphology. It exhibits a dominant, bright central bulge, characterized by a yellowish-orange hue, which likely indicates an older stellar population. There is an absence of prominent spiral arms or a distinct disk structure. The galaxy's overall color suggests a relatively low ongoing star formation rate. There might be some minor disturbances or tidal features in the surrounding area, hinting at a possible past interaction or merger event, although the dominant impression is of a relaxed, relatively undisturbed system. The galaxy’s shape is mostly round, versus cigar shaped.
