The object appears to be a spiral galaxy at a non-negligible redshift. It exhibits a distinct disk structure with observable spiral arms. The arms appear somewhat flocculent. The central bulge is prominent, displaying a color gradient consistent with an older stellar population. There is evidence of ongoing star formation within the spiral arms, indicated by bluer regions. A bar-like structure seems to transect the bulge region along its major axis. There might be a minor disturbance that indicates a potential tidal interaction or minor merger, but the galaxy itself appears to be relatively undisturbed, with clearly defined spiral arms and a noticeable bulge. The galaxy presents a moderate inclination relative to our line of sight.
