In this paper, we reconstruct an [Formula: see text] function from [Formula: see text]CDM model and obtained field equations for this function [Formula: see text] in a flat FLRW viscous-fluid dusty universe, where [Formula: see text] is the torsion scalar, [Formula: see text] is an arbitrary constant and [Formula: see text] is the cosmological constant. We have solved the field equations and obtained an scale factor [Formula: see text] with [Formula: see text] as an integrating constant and [Formula: see text] is an arbitrary constant generated from viscous fluid, and this type of scale factor gives a time-dependent deceleration parameter. We have made observational constraints on Hubble parameter [Formula: see text] and apparent magnitude [Formula: see text] with observational datasets [Formula: see text] data and SNe Ia data by applying [Formula: see text]-test, to obtain the best-fit values of model parameters. Using these values of cosmological parameters, we have discussed our model results. We have obtained a transit phase accelerating quintessence dark energy model in viscous-fluid universe with effective equation of state ([Formula: see text]).