The galaxy presents as a spiral galaxy with a moderate bulge. Two prominent spiral arms are observed, loosely wound around the central bulge, giving it a barred appearance. The disk is not edge-on, and the spiral arms appear somewhat patchy, which indicates moderate star formation. Some minor disturbances can be seen in the spiral arms, likely due to past minor merger events or interactions. There is no central merging visible. Overall, the galaxy appears to be in a relatively settled state with ongoing star formation.
