Intermediate Mass Black Holes (IMBHs) are of particular interest as they are filling the gap between stellar mass BHs and supermassive BHs. Recently, the "Microscopic Theory of Black Hole, MTBH" was suggested by Ter-Kazaryan(2001). This theory explores a spontaneous breaking of gravitational gauge symmetry at huge energies, and thereof for that of rearrangement of vacuum state. Aiming to utilize the MTBH in investigating the feasibility of IMBH over several domains, 100 configurations were simulated with a dedicated existing FORTRAN code. IMBHs' parameters were computed in order to obtain all the integral physical characteristics. The simulation were performed for masses ranges from M = 44.4 - 9.60x10° Mo. The integrated parameters are the BH mass, the total number of particles, the gravitational packing coefficients, the density and pressure profiles and the gravitational radius was obtained. Then the stabilities of these configurations over the specified domains were examined.