The galaxy presents as a grand design spiral, viewed face-on. A central bulge is visible, appearing relatively small and not significantly dominant. Flocculent spiral arms emanate from the central region, exhibiting a moderately wound morphology. Multiple spiral arms can be discerned, but the exact count is somewhat ambiguous due to their diffuse nature and overlapping structure. The arms are populated by numerous bright knots of star formation regions, evident as localized blueish concentrations, suggesting active stellar birth. The disk component of the galaxy appears extensive, with the spiral arms extending outwards. No significant bar structure is immediately apparent at the resolution of the image, and no prominent tidal features or signs of a major ongoing merger are visible, though some minor disturbances within the spiral arms may indicate past interactions or internal processes. The overall structure suggests a relatively well-defined and undisturbed spiral galaxy morphology.
