This galaxy appears to be a spiral galaxy, observed at a redshift indicating a considerable distance. The galaxy is tilted relative to our line of sight, presenting a disk-like structure. While the disk is not perfectly edge-on, it isn't entirely face-on either. There is evidence of spiral arm structure, though the arms appear somewhat flocculent and not particularly tightly wound. The central bulge is moderately prominent, exhibiting a yellowish hue indicative of an older stellar population. The disk shows a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. Overall, the galaxy exhibits signs of active star formation. There are no readily apparent signs of major merging activity, though minor disturbances cannot be ruled out. It appears to be a relatively massive system.
