The galaxy presents as a face-on spiral, exhibiting a relatively high degree of rotational symmetry. The arms display a somewhat flocculent morphology, not sharply defined but rather patchy. The winding of the arms is moderate, neither tightly wound nor overly open. Star formation appears to be active within the spiral arms, as evidenced by the blue color, suggestive of a young stellar population.

A central bulge is discernible but not particularly prominent, appearing relatively small compared to the overall disk size. There may be a weak bar-like structure oriented across the center, though the evidence for this is not definitive. There are 2 main spiral arms that are clearly visible.

Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger event. However, minor tidal features or distortions might be present upon closer inspection.
