  We investigate the near horizon geometry of the simplest representative of
the class of axisymmetric space-times: the Kerr Vaidya metrics. Kerr Vaidya
metrics can be derived from the Vaidya metric by the complex coordinate
transformation suggested by Newman and Janis. We show that the energy momentum
tensor belongs to type 3 in the Segre Hawking Ellis classification but has a
special form with all Lorentz invariant eigenvalues belonging to zero. We find
a location of the apparent horizon for quasi-stationary Kerr Vaidya black
holes. The energy-momentum tensor of the Kerr Vaidya geometries violates the
null energy condition. We show that energy density, pressure, and flux for an
infalling observer are diverging in the outgoing Kerr Vaidya metric. This
firewall leads to the violation of a specific quantum energy inequality.
