We study the processes gamma e --> gamma e and gamma gamma --> gamma gamma,
in the context of the proposal for Weak Scale Quantum Gravity (WSQG) with
large extra dimensions. With an ultraviolet cutoff M-S similar to 1 TeV for
the effective gravity theory, the cross sections obtained for these proces
ses at the Next Linear Collider (NLC), with the e gamma an gamma gamma opti
ons, deviate from the predictions of the Standard Model significantly. Our
results suggest that, for typical proposed NLC energies and luminosities, t
he predictions of WSQG can be tested in the range 1 TeV less than or simila
r to M-S less than or similar to 10 TeV, making e gamma an gamma gamma coll
iders important tools for probing WSQG.