The galaxy presents as a spiral type, characterized by a prominent disk structure. Within the disk, spiral arms are discernable, exhibiting a two-armed morphology. The spiral arms appear tightly wound. A central bulge is visible, representing approximately half the extent of the galaxy, and an indication of a bar structure crossing the galaxy's central region is visible. Star formation is occurring throughout the galaxy. The overall appearance suggests a system undergoing some sort of interaction as it looks slightly disturbed.
