The galaxy exhibits a clear disk structure with a prominent bulge at its center. The disk is not perfectly circular, displaying a slight ellipticity. Faint spiral arm structures are suggested within the disk, though they are not sharply defined. The central bulge appears to be a yellowish hue, potentially indicating a population of older stars. The overall color gradient suggests ongoing star formation within the disk, particularly in regions with a bluer tint. The galaxy's orientation is close to face-on, providing a relatively unobstructed view of its morphology. No signs of major disturbances such as strong tidal tails or obvious merger activity are apparent, although there may be some minor irregularities in the outer disk.
