  NRAO 150 -a compact and bright radio to mm source showing core/jet structure-
has been recently identified as a quasar at redshift z=1.52 through a near-IR
spectral observation. To study the jet kinematics on the smallest accessible
scales and to compute the first estimates of its basic physical properties, we
have analysed the ultra-high-resolution images from a new monitoring program at
86 GHz and 43 GHz with the GMVA and the VLBA, respectively. An additional
archival and calibration VLBA data set, covering from 1997 to 2007, has been
used. Our data shows an extreme projected counter-clock-wise jet position angle
swing at an angular rate of up to ~11 deg./yr within the inner ~31 pc of the
jet, which is associated with a non-ballistic superluminal motion of the jet
within this region. The results suggest that the magnetic field could play an
important role in the dynamics of the jet in NRAO 150, which is supported by
the large values of the magnetic field strength obtained from our first
estimates. The extreme characteristics of the jet swing make NRAO 150 a prime
source to study the jet wobbling phenomenon.
