The galaxy presents as a spiral type, observed at a redshift indicating significant distance. It exhibits a moderate inclination relative to our line of sight, allowing a partial view of its disk structure. Prominent spiral arms are evident, displaying a somewhat flocculent morphology. These arms appear relatively well-defined and extend outwards from a central bulge region. The bulge itself appears of moderate size, neither dominating nor insignificant in comparison to the disk. 

There may be a weak bar feature present, but it is indistinct. The overall colour of the galaxy suggests ongoing star formation, particularly within the spiral arms. The structure of the galaxy does not appear significantly disturbed, with no strong visual indications of a recent major merger. However, some minor irregularities in the arm structure are visible, perhaps indicative of minor interactions or internal dynamical processes.
