  We study gravitational lensing by a recently proposed black hole solution in
Loop Quantum Gravity. We highlight the fact that the quantum gravity
corrections to the Schwarzschild metric in this model evade the `mass
suppression' effects (that the usual quantum gravity corrections are
susceptible to) by virtue of one of the parameters in the model being
dimensionless, which is unlike any other quantum gravity motivated parameter.
Gravitational lensing in the strong and weak deflection regimes is studied and
a sample consistency relation is presented which could serve as a test of this
model. We discuss that though the consistency relation for this model is
qualitatively similar to what would have been in Brans-Dicke, in general it can
be a good discriminator between many alternative theories. Although the
observational prospects do not seem to be very optimistic even for a galactic
supermassive black hole case, time delay between relativistic images for
billion solar mass black holes in other galaxies might be within reach of
future relativistic lensing observations.
