The galaxy presents as a spiral system with a prominent disk structure. Spiral arms are clearly visible and exhibit a tightly wound morphology. The central bulge appears relatively small compared to the overall disk size. Color gradients suggest a mix of stellar populations, with the central bulge exhibiting a more yellow-red hue, indicative of older, cooler stars, whereas the disk shows bluer regions, possibly associated with ongoing star formation. The galaxy does not show any clear signs of major mergers, though there may be minor irregularities in the disk, potentially due to minor gravitational disturbances. Overall, the galaxy appears as a well-defined spiral galaxy with a relatively compact central region.