The galaxy exhibits a distinct spiral morphology, presented at an almost edge-on inclination relative to our line of sight. Its disk is characterized by well-defined spiral arms. The spiral arms appear tightly wound. A bar structure is evident traversing the central bulge, which extends from the main part of the galaxy, with the majority of the galaxy being lit by the bulge. The center of the galaxy exhibits a yellow glow with dusty patches, suggestive of older stellar populations or obscuring dust lanes. Overall, the spiral arms appear quite symmetrical and relatively undisturbed.
