This galaxy exhibits characteristics consistent with a spiral morphology. A central bulge is present, though not particularly dominant, surrounded by a disk structure. The spiral arms are quite pronounced, and are tightly wound around the galactic center. A hint of a bar structure is visible in the inner regions of the disk. The colors suggest ongoing star formation, especially in the disk, with bluer regions indicating the presence of young, hot stars. There is no strong visual indication of a major merger, but minor disturbances might be present. The galaxy is not viewed perfectly edge-on; rather it is at an oblique angle to our line of sight. Overall, this galaxy presents a fairly well-defined spiral structure with active star formation and a small to moderate bulge.
