The galaxy presents a flattened, disk-like morphology, indicative of a spiral or lenticular classification. It is observed at a moderate inclination, revealing the spiral structure. The central bulge appears relatively small in proportion to the overall disk size. Distinct spiral arms are present, displaying a tightly wound structure that suggests a grand-design spiral galaxy. Patches of star formation and dust lanes are observed along the spiral arms, indicating active regions of ongoing stellar birth. The galaxy exhibits a smooth texture, with limited morphological peculiarities. There is no obvious presence of a strong bar feature. The overall color of the galaxy suggests a mix of stellar populations, with a central yellowish hue indicative of older stars in the bulge, and bluer hues in the spiral arms representing younger, hotter stars. The galaxy is well-defined and exhibits clear, discernible structure.
