  We construct a relativistic model for the newly discovered millisecond pulsar
PSR J0514 - 4002A located in the globular cluster NGC 1851 (A. Ridolfi, P.C.C.
Freire, Y. Gupta, S.M. Ransom, MNRAS 490, 3860 (2019)) by using Tolman VII
spacetime. We have obtained central density ($\rho_{0}$), central pressure
($p_{0}$), probable radius, compactness ($u$) and surface redshift ($Z_{s}$) of
the above mentioned newly discovered millisecond pulsar, which is very much
consistent with reported data. Equation of State (EoS) of the millisecond
pulsar has comes out as stiff in nature which is physically acceptable. Not
even that our proposed model can analyze most of the millisecond pulsars having
masses up to $1.51 M_{\odot}$.
