  The anisotropic Bianchi type I in multi-scalar field cosmology is studied
with a particular potential of the form $\rm V= V_0 e^{-\left[\lambda_1 \phi_1
+ \cdots + \lambda_n \phi_n \right]}\,,$ which emerges as a condition between
the time derivatives of their corresponding momenta. Using the Hamiltonian
formalism for the inflation epoch with a quintessence framework we find the
exact solutions for the Einstein-Klein-Gordon (EKG) system with different
scenarios specified by the parameter $\rm \lambda^2= \sum_{i=1}^n \lambda_i^2$.
For the quantum scheme of this model, the corresponding Wheeler-DeWitt (WDW)
equation is solved by applying an appropriate change of variables and suitable
ansatz.
