The galaxy exhibits a prominent spiral structure. Two well-defined spiral arms emanate from the central bulge region. The arms appear relatively tightly wound. The central bulge displays a moderate size relative to the overall galactic disk. There is no apparent bar structure. The galaxy appears to be undergoing moderate star formation activity. The galaxy shows no signs of major mergers, however, there is a clear asymmetry with what appears to be possible minor disturbances or tidal distortion in the spiral arms, potentially indicating a minor interaction or past interaction.
