  We performed VLBA observations of the Broad Absorption Line Quasar
FIRST\,J155633.8+351758, "the first radio loud BALQSO". Our observations at
15.3 GHz partially resolved a secondary component at positional angle (PA)
$\approx 35^{\circ}$. We combine this determination of the radio jet projection
on the sky plane, with the constraint that the jet is viewed within
$14.3^{\circ}$ of the line of sight (as implied by the high variability
brightness temperature) and with the position angle (PA) of the optical/UV
continuum polarization in order to study the quasar geometry. Within the
context of the standard model, the data indicates a "dusty torus" (scattering
surface) with a symmetry axis tilted relative to the accretion disk normal and
a polar broad absorption line outflow aligned with the accretion disk normal.
We compare this geometry to that indicated by the higher resolution radio data,
brightness temperature and optical/UV continuum polarization PA of a similar
high optical polarization BALQSO, Mrk\,231. A qualitatively similar geometry is
found in these two polar BALQSOs; the continuum polarization is determined
primarily by the tilt of the dusty torus.
