Turbulence is ubiquitous in astrophysical fluids such as the interstellar medium and intracluster medium. To maintain turbulent motion, energy must be injected into the fluids. In turbulence studies, it is customary to assume that the fluid is driven on a scale, but there can be many different driving mechanisms that act on different scales in astrophysical fluids. We expect different statistical properties of turbulence between turbulence with single driving scale and turbulence with double driving scales. In this work, we perform 3-dimensional incompressible MHD turbulence simulations with energy injection in two ranges, 2<k< ${surd}$12 (large scale) and 15<k<26 (small scale). We separated into two parts, which are fixed large scale driving and fixed small scale driving. In case of fix large scale driving, two peaks appear in kinetic energy spectrum when the energy injection rate on small scale are comparable to that on large scale. On the other hands, in case of fixed small scale driving we can find two peaks even the energy injection rate on large scale is much smaller that that on small scale. On time evolution of magnetic energy densities in fixed small scale driving case, there seems to be a threshold of energy injection rate.