This galaxy exhibits a prominent disk structure with distinct spiral arm morphology. The spiral arms appear tightly wound in the inner region, transitioning to a more medium winding configuration in the outer regions. Two distinct spiral arms are visible. A significant bar structure is observed across the central region of the galaxy, extending from the core. The bulge is moderate in size, compared to the overall disk. The disk appears largely undisturbed, with no strong evidence of major mergers or interactions, although some minor disturbances cannot be ruled out. Overall, the galaxy presents as a classical barred spiral galaxy.
