  We simulate forced quasi-static magnetohydrodynamic turbulence and
investigate the anisotropy, energy spectrum, and energy flux of the flow,
specially for large interaction parameters ($N$). We show that the angular
dependence of the energy spectrum is well quantified using Legendre
polynomials. For large $N$, the energy spectrum is exponential. Our direct
computation of energy flux reveals an inverse cascade of energy at low
wavenumbers, similar to that in two-dimensional turbulence. We observe the flow
be two-dimensional (2D) for moderate $N$ ($N \sim 20$), and two-dimensional
three-component (2D-3C) type for $N \ge 27$. In our forced simulation, the
transition from 2D to 2D-3C occurs at higher value of $N$ than Favier et al.,
["On the two-dimensionalization of quasistatic magnetohydrodynamic turbulence,"
Phys. Fluids 22, 075104 (2010)] who employ decaying simulations.
