  We investigate the phase space of a scalar field theory obtained by
minisuperspace deformation. We consider quintessence or phantom scalar fields
in the action which arise from minisuperspace deformation on the
Einstein-Hilbert action. We use a modified Poisson Algebra where Poisson
brackets are the $\alpha$-deformed ones and are related to the Moyal-Weyl star
product. We discuss early and late-time attractors, and we reconstruct the
cosmological evolution. We show that the model can have $\Lambda$CDM model as a
future attractor if we initially consider a massless scalar field without a
cosmological constant term.
