The object presents as a spiral galaxy of intermediate redshift. The core is relatively small and indistinct, appearing as a slight brightening in the center of the disk. The spiral arms are somewhat loosely wound and display clumpy structures, possibly indicating active star formation regions. The overall color is bluer, suggesting a population of young, hot stars. There appears to be minor asymmetry in the morphology, potentially indicating a past or ongoing minor interaction or disturbance. No obvious strong tidal features are visible, however. The galaxy exhibits an average angular size. There appears to be a slightly disturbed morphology.
