  The effective quantum dynamics of Bianchi I spacetime is addressed within the
statistical regularization scheme in Quantum Reduced Loop Gravity. The case of
a minimally coupled massless scalar field is studied and compared with the
effective $\bar{\mu}-$Loop Quantum Cosmology. The dynamics provided by the two
approaches match in the semiclassical limit but differ significantly after the
bounces. Analytical and numerical inspections show that energy density,
expansion scalar and shear are bounded also in Quantum Reduced Loop Gravity and
the classical singularity is resolved for generic initial conditions in all
spatial directions.
