Amorphous radio source in Ophiuchus alongside a potential synthetic analog. Left: MeerKAT image with a robust −1.0 weighting rotated 41° clockwise to align the jet on the y axis. Right: Snapshot from the numerical simulations of Upreti et al. (2024) showing the integrated synchrotron intensity at 1.28 GHz of a relativistic jet undergoing kink instability. The panel spans 50 kpc × 120 kpc. Similar features in the observations and simulations are labeled.