The galaxy presents a prominent disk structure, observed at a moderate inclination. Spiral arms are clearly visible, emanating from a central bulge. The arms appear tightly wound, exhibiting a grand design morphology. Dust lanes are discernible within the spiral arms, contributing to a mottled appearance. The central bulge appears relatively small compared to the overall disk size. There is no strong evidence of a bar structure. Based on visual inspection, the galaxy does not show obvious signs of major mergers or significant tidal disturbances, though some minor irregularities in the disk structure may be present. The color gradient suggests a population of younger, bluer stars present within the spiral arms, while the central bulge exhibits a more yellow/red hue, indicative of an older stellar population.
