The galaxy presents as a spiral type, exhibiting a prominent central bulge and a disk component. The spiral arms appear tightly wound and are somewhat indistinct, making it challenging to discern a precise arm count. The disk shows evidence of features or structures beyond a smooth appearance. There is no apparent bar structure. The bulge seems to be a moderate to small fraction of the galaxy. The image does not clearly indicate a major merger event, however there is a possibility of a minor disturbance.
