This galaxy exhibits a prominent disk structure. Evident spiral arm features are present, displaying a somewhat flocculent morphology. A central bulge is visible; it appears to be of moderate size, but it doesn't dominate the galaxy's overall structure. There is some evidence of a bar-like structure within the central region, extending outward from the bulge. The color distribution suggests ongoing star formation within the spiral arms, as indicated by the presence of bluer regions. Overall, the galaxy appears relatively undisturbed, lacking strong signs of major merger activity. There might be minor disturbances present in the disk structure. The galaxy displays a significant disk component with well-defined spiral arms.