The galaxy presents as a spiral type, exhibiting a discernible disk structure. The spiral arms appear loosely wound and are well-defined. A central bulge is either small or non-existent. The galactic disk shows evidence of active star formation, indicated by blue regions along the spiral arms. There are luminous red areas indicating the existence of older stars, potentially from a disrupted star formation process. There appears to be some type of interaction or disturbance affecting the morphology, but it is hard to say what it is. There is no central bar that can be discerned. The galaxy is generally blue-shifted, meaning it is either moving towards us, or is undergoing relatively rapid star formation.