The structure of light quark star is studied within a new two-flavor NJL model. By retaining the contribution from the vector term in the Fierz-transformed Lagrangian, a two-solar-mass pure quark star is achieved. To overcome the disadvantage of three-momentum truncation in the regularisation procedure, we introduce the proper-time regularisation. We also employ the newly proposed definition of vacuum pressure [29], in which the quasi-Wigner vacuum (corresponding to the quasi-Winger solution of the gap equation) is used as the reference ground state. Free parameter includes only a mixing constant α which weighs contribution from Fierztransformed Lagrangian. We constrain α to be around 0.9 by the observed mass of pulsars PSRJ0348+0432 and PSRJ1614 − 2230. We find the calculated surface energy density meets the requirement (> 2.80 × 10 14 g/cm 3 ) [28]. Besides, for a 1.4 solar mass star, the tidal Love number k 2 and deformability Λ are calculated which satisfies the constrain 200 < Λ < 800 [31,35,41].