The galaxy presents a spiral morphology, exhibiting a prominent disk structure. The arms appear loosely wound. There is evidence of a bar feature crossing the central bulge region. The bulge itself is of moderate size compared to the disk.  The overall color suggests ongoing star formation within the disk, with a redder bulge. There appears to be some minor disturbance present indicating a possible past interaction or merger event. The galaxy exhibits a relatively face-on orientation. The galaxy appears to have two dominant spiral arms.
