The galaxy presents a clear spiral structure. The spiral arms are prominent, with a morphology that appears neither tightly wound nor exceptionally loose, suggesting an intermediate winding pattern. The overall disk component dominates the galaxy's appearance.

The galaxy does not appear to be strongly barred, with only a hint of a weak bar-like structure possibly present. The central bulge is relatively prominent and of moderate size, but does not dominate the overall light profile. 

The color distribution across the galaxy shows a noticeable gradient, the central bulge showing a more yellow appearance than the outer disk and spiral arms. The bluer light observed in the spiral arms is indicative of active star formation. There is no obvious sign of major ongoing mergers or tidal disturbances.
