The galaxy presents as a slightly inclined spiral, exhibiting well-defined spiral arms. The morphology suggests a dominant disk structure with a small to moderate bulge component. There's no sign of a galactic bar. The arms are grand design type. The galaxy appears relatively undisturbed, showing no obvious signs of major merging activity. The colour profile indicates a mixture of stellar populations, with a yellower central bulge, suggesting older stars, and bluer spiral arms, indicative of ongoing star formation. The galaxy shows a relatively high degree of spiral structure.