  Methods. We performed measurements of the \MgII, \MgI, \FeIIa, \FeIIb, and
\FeIIc\ spectral lines present in the spectra of the selected sample to
determine the EW and velocity of the flows observed in the star-forming
galaxies. Subsequently, we conducted $10^7$ bootstrap simulations using
Spearman's rank correlation coefficient ($\rho_s$) to explore correlations with
galaxy properties. Furthermore, we calculated the covering factor, gas density,
and optical depth for the measured \ion{Fe}{II} doublets.
  Results. Our analysis revealed strong correlations between the EW of
\ion{Mg}{II} lines and both $M_{*}$ ($\rho_s=0.43$, 4.5$\sigma$) and SFR
($\rho_s=0.42$, 4.4$\sigma$). For the \ion{Fe}{II} lines, we observed strong
correlations between the EW and SFR ($\rho_s\sim0.65$, $>3.9\sigma$), with a
weaker correlation for $M_{*}$ ($\rho_s\sim0.35$, $>1.9\sigma$). No notable
correlations were found between velocity measurements of \ion{Mg}{II} line and
$M_{*}$, SFR, or sSFR of the objects ($\rho_s\sim0.1)$. However, a negative
strong correlation was found between the velocity of the \ion{Fe}{II} lines and
the SFR of the galaxies ($\rho_s\sim-0.45$, $\sim3\sigma$). Our results align
with previous studies but studying FIR-selected objects. Finally, we detected a
candidate \textit{loitering outflow}, a recently discovered subtype of FeLoBAL
quasar, at redshift of $z=1.4399$, exhibiting emission in \ion{C}{III}] and low
line velocities ($|v|\lesssim$ 200 km/s).
