  We examine the scaling laws of MHD turbulence for three different types of
forcing functions and imposing at all times the four-fold symmetries of the
Taylor-Green (TG) vortex generalized to MHD; no uniform magnetic field is
present and the magnetic Prandtl number is equal to unity. We also include a
forcing in the induction equation, and we take the three configurations studied
in the decaying case in [E. Lee et al. Phys. Rev.E {\bf 81}, 016318 (2010)]. To
that effect, we employ direct numerical simulations up to an equivalent
resolution of $2048^3$ grid points. We find that, similarly to the case when
the forcing is absent, different spectral indices for the total energy spectrum
emerge, corresponding to either a Kolmogorov law, an Iroshnikov-Kraichnan law
that arises from the interactions of turbulent eddies and Alfv\'en waves, or to
weak turbulence when the large-scale magnetic field is strong. We also examine
the inertial range dynamics in terms of the ratios of kinetic to magnetic
energy, and of the turn-over time to the Alfv\'en time, and analyze the
temporal variations of these quasi-equilibria.
