The galaxy presents a clear spiral morphology. The spiral arms are well-defined and extend noticeably from a central bulge. The arms appear relatively tightly wound. A bar structure is visible across the central bulge, which seems moderately sized relative to the disk. The galaxy is not perfectly edge-on, but is observed at a slight angle, enabling clear observation of spiral features. No obvious signs of recent merger events are visible. Star formation appears to be occurring within the galaxy, as indicated by the slightly blue tint.
