The galaxy presents a primarily smooth morphology, with a significant fraction of light concentrated in a central region. The galaxy appears elongated, not perfectly spherical. There is a subtle suggestion of a disk-like structure, though the dominant impression is one of smoothness, lacking prominent spiral arms or bar features. There may be minor disturbances indicating gravitational interactions, but they don't appear to be experiencing a full-blown merger. The color indices suggest relatively evolved stellar populations. The inferred mass is on the higher end. Star formation rates indicate a relatively quiescent galaxy, with lower specific star formation rate.
