The galaxy presents as a spiral with a noticeable disk structure. Spiral arms are visible, displaying a tightly wound morphology. The color profile suggests active star formation. A central bulge is present, though it appears to be relatively small. There's a possible bar feature bisecting the bulge. The disk exhibits a high degree of symmetry, lacking obvious signs of major tidal disruption or ongoing merger activity. The spiral arms have a distinct blue tint indicating the likely presence of young, hot stars. The bulge, in contrast, displays a yellower hue, suggesting an older stellar population. The overall shape is moderately elliptical. The image suggests that the galaxy is a spiral galaxy with tightly wound arms, a small bulge, and ongoing star formation.