This galaxy appears to be a spiral galaxy at a considerable distance, exhibiting a redshift indicative of its cosmological recession. The galaxy presents a relatively well-defined disk structure with prominent spiral arms. These arms are not tightly wound, displaying a more open, grand-design morphology. Evidence suggests two dominant spiral arms are present.

A central bulge is noticeable, appearing moderately sized relative to the disk. The galactic bar structure is not strongly pronounced. The galaxy appears relatively isolated, without any clear signs of major interactions or mergers, though some minor disturbances cannot be ruled out. The color indices suggest ongoing star formation, with a bluer color in the disk compared to the central bulge.
