  $f(Q)$ symmetric-teleparallel gravity is considered in view of Quantum
Cosmology. Specifically, we derive cosmological equations for $f(Q)$ models and
then investigate the related energy conditions. In the minisuperspace
formalism, the point-like $f(Q)$ Hamiltonian is taken into account. In this
framework, we obtain and solve the Wheeler-De Witt equation, thus finding the
Wave Function of the Universe in different cases. We show that the Hartle
Criterion can be applied and classical observable universes occur.
