This galaxy exhibits a prominent spiral structure. The arms appear loosely wound and are traced by regions of active star formation, evidenced by their bluer color relative to the galactic bulge. A significant, moderately sized bulge dominates the central region, displaying a yellowish hue, which suggests a population of older stars. A bar structure is observed, extending through the central region of the galaxy, though it is neither a very strong nor very weak bar. Based on the disturbances, this galaxy is not actively merging. It appears to be undisturbed with a small number of merging disturbances. The morphology suggests this is a non-smooth galaxy, but rather a galaxy that includes features such as a disk with arms.
