[12] There is a presence of a compact core displaying strong increase of flux density[13] with the outermost component being separated into several smaller regions enveloped completely by emission.

[16] With an estimated length of 300 kiloparsecs, this makes the longest one detected so far in any of the high redshift quasars.

[17] Advanced CCD Imaging Spectrometer also revealed a complex structure in the X-ray jet from the core with bright knots of different morphologies.

Upon reaching 18 arcseconds from the core, the jet suddenly bends slightly causing the re-brightening of radio emission.

In additional, there is a 90° rotation of the magnetic field suggesting it might be compressed to the plane that is found perpendicular to the axis.