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

On the Possible Spacetime Structures of Rotating Loop Quantum Black Holes