This galaxy exhibits a flattened, disk-like morphology viewed approximately edge-on. A central bulge is visible, appearing relatively smooth and concentrated. The disk appears slightly warped or disturbed. The color is primarily blue, with a hint of a yellow center. Based on the color and morphology, the disk is likely a site of ongoing star formation, while the central bulge is a population of older stars. There is no evidence of a major ongoing merger or significant tidal disturbances. The galaxy has a moderate amount of star formation, but does not appear to be a strong starburst galaxy. There are subtle color variations across the disk, with the outer regions appearing bluer and the inner regions gradually transitioning to a yellow hue. This suggests a radial gradient in the stellar populations, with younger, bluer stars dominating the outer disk and older, redder stars concentrated in the bulge and inner disk.
