The galaxy exhibits a distinct spiral morphology. Two prominent spiral arms emanate from the central region, displaying a tightly wound structure. The central bulge appears relatively small in comparison to the disk, showing moderate size. There is evidence of a weak bar structure extending across the central region. The disk appears to be viewed close to face-on.

Color gradients are visible across the galaxy, with a bluer hue in the spiral arms and a redder hue toward the bulge, suggesting a distribution of stellar populations where younger, hotter stars are more prominent in the arms. The overall structure suggests a relatively high star formation rate and a substantial mass. There appears to be no ongoing major merging activity, however, minor disturbances may exist within the spiral structure.