We present the temporal and spectral study of blazar PKS 0208-512, using recent flaring activity from November 2019 to March 2020, as detected by Fermi-LAT, Swift-XRT/UVOT observatories. The source was in a low ${gamma}$-ray flux state for a decade and started flaring in November 2019, which continues until March 2020. During the activity state, 2-days binned ${gamma}$-ray lightcurve shows multiple-peaks indicating sub-flares. To understand the possible physical mechanisms behind flux enhancement, a detailed temporal and spectral study has been carried out by dividing the activity into several flux-states. Timing analysis of lightcurves suggests that peaks of sub-flares have rise and decay time in days-order with flux-doubling time $sim$ 2-days. The 2-days binned ${gamma}$-ray lightcurve shows double-lognormal flux distribution. The broadband spectral energy distribution for three selected flux states can be well fitted under synchrotron, synchrotron-self-Compton (SSC) and external-Compton (EC) emission mechanisms. We obtained the physical parameters of the source and their confidence intervals through ${chi}^2$-statistics. Our spectral study suggests that during quiescent-state, gamma-ray spectrum can be well explained by considering the EC-scattering of IR-photons from the dusty-torus. However, gamma-ray spectra corresponding to flares demand additional target photons from broad-line-region (BLR) along with the IR. These suggest that during flares, the emission-region is close to the edge of BLR, while for quiescent-state the emission-region is away from the BLR. The best-fit results suggest that, marginal increase in the magnetic-field can result in the flux enhancement. This is possibly associated with the efficiency of particle acceleration during flaring-states as compared to quiescent-state.
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