  To date, a mathematically consistent construction of effective rotating black
hole models in the context of Loop Quantum Gravity (LQG) is still lacking. In
this work, we start with the assumption that rotating LQG black hole metrics
can be effectively obtained using Newman-Janis Algorithm. Then, based on a few
extra fair assumptions on the seed metric functions, we make a conjecture on
what a rotating LQG black hole would generically look like. Our general
arguments and conclusions can be supported by some known specific examples in
the literature.
