This galaxy presents as a face-on spiral, exhibiting a disk structure with well-defined spiral arms. These spiral arms are prominent and show a loosely wound morphology, extending outwards from a central region. The color of the arms indicates a substantial presence of relatively young, hot stars, contributing to a bluish hue.

The galaxy's central region appears diffuse and somewhat concentrated, suggesting a modest bulge. The light from this region is generally redder than the spiral arms, which could be indicative of an older stellar population. The spiral arms are not perfectly symmetrical, exhibiting some degree of irregularity and patchiness, which may be due to ongoing star formation. There are no obvious signs of a strong bar structure.

The overall structure shows no obvious signs of tidal disturbances or recent major mergers; however, some minor irregularities in the arm structure could suggest past interactions or internal dynamical processes.
