The galaxy presents as a flattened, elongated structure with a noticeable central bulge. The color gradient indicates a concentration of older stellar populations toward the center, exhibiting a yellowish to orange hue, likely indicative of a greater proportion of red giant stars. The outer regions of the galaxy display a bluer tint, possibly suggesting ongoing star formation within the disk, although these regions are not well-resolved in the image. There is some subtle patchiness along the disk. The morphology of the galaxy appears to be that of a disk galaxy, although some minor disturbances and distortions are observed, perhaps from an earlier merging event. Overall, the galaxy appears to be a relatively massive system.
