  In this article, we demonstrate that PKSJ 1037-2705 has a weak accretion flow
luminosity, well below the Seyfert1/QSO dividing line, weak broad emission
lines (BELs) and moderately powerful FRII extended radio emission. It is one of
the few documented examples of a broad-line object in which the time averaged
jet kinetic luminosity, $\bar{Q}$, is larger than the total thermal luminosity
(IR to X-ray) of the accretion flow, $L_{bol}$. The blazar nucleus dominates
the optical and near ultraviolet emission and is a strong source of hard
X-rays. The strong blazar emission indicates that the relativistic radio jet is
presently active. The implication is that even weakly accreting AGN can create
powerful jets. Kinetically dominated ($\bar{Q}>L_{bol}$) broad-line objects
provide important constraints on the relationship between the accretion flow
and the jet production mechanism.
