The galaxy appears to be a spiral galaxy with a prominent disk structure. The spiral arms are clearly visible, exhibiting a somewhat flocculent, rather than grand design, morphology. There is a moderate central bulge, with a gradual transition into the disk. The arms are traced by regions of bluer light, suggesting ongoing star formation. The overall color of the galaxy indicates an intermediate age stellar population. There is no obvious sign of a bar structure. Some minor irregularities within the disk suggest possible minor interactions or disturbances.
