  We study the spectro-polarimetric properties of a newly discovered black hole
X-ray binary Swift\,J151857.0-572147 jointly using {\it IXPE} and {\it NuSTAR}
observations during March 2024. The analysis of {\it IXPE} data reports
mode-independent polarization degree (PD) $1.34\pm0.27$ and polarization angle
(PA) $-13.69^\circ\pm5.85^\circ$, while the model-dependent analysis gives PD
$1.18\pm0.23$ and PA $-14.01^\circ\pm5.80^\circ$. The joint spectral analysis
of the broadband data and {\it NuSTAR} analysis in isolation constrain the mass
of the central black hole between $\sim 9.2\pm1.6-10.5\pm1.8 M_\odot$ and a
moderate spin parameter of $\sim0.6\pm0.2-0.7\pm0.2$ with disk inclination
$\sim 38^\circ\pm9^\circ-47^\circ\pm15^\circ$. The power-law photon index and
cutoff energy are $2.27\pm0.03-2.42\pm0.05$ and $\sim 40\pm7-62\pm8$ keV,
suggesting a transition to the soft spectral state of the source during the
observation period. Additionally, the best-fitted halo mass accretion is less
compared to the disk mass accretion rate, and a relatively lower corona size of
6-9 r$_g$ indicates the same spectral state. The mass outflow rate was also low
($<3$\% $\dot M_{\rm Edd}$) during these epochs. The hydrogen column density
obtained from the fit is relatively high $\sim 4-5\times 10^{22}$ cm$^{-2}$.
