This galaxy presents as a spiral, exhibiting a prominent disk structure. The spiral arms are relatively tightly wound. Two main arms are clearly discernable, showing a fairly symmetrical pattern. The light distribution suggests a moderate-sized bulge in the galaxy's center. The overall color of the disk indicates a substantial population of young, blue stars, suggesting ongoing or recent star formation. No significant signs of a major merger are apparent, although there might be a minor disturbance in the galaxy's morphology. The galaxy is not oriented edge-on; we observe it at an angle that allows us to see the spiral structure.
