The galaxy presents a clear spiral structure. The arms are tightly wound around a prominent central bulge that emits a significant amount of light. The spiral arms are well-defined, exhibiting a multi-armed morphology, possibly with three or more arms discernible. The galaxy is not perfectly face-on, presenting a slight inclination to our line of sight. There's a hint of a bar structure extending through the central region, but it's not highly pronounced. There's no immediate visual evidence of a major ongoing merger, but some minor disturbances or asymmetries might be present. The arms exhibit some flocculent structure, suggesting regions of active star formation.
