This galaxy appears to be a spiral galaxy, exhibiting a disk-like structure with indications of spiral arm morphology. The arms are not sharply defined, presenting a somewhat flocculent appearance. Color gradients suggest ongoing star formation within the spiral arms, particularly in localized regions of bluer light. A central bulge is visible with a moderate size compared to the disk, displaying a yellowish hue suggestive of an older stellar population. The galaxy shows no obvious signs of major mergers or tidal disturbances, and appears relatively isolated and undisturbed. There is likely a bar structure within the central region of the disk. Overall, the galaxy exhibits a classic spiral structure with a well-defined disk, a moderate bulge, and indications of active star formation within its spiral arms.
