  In this work we present the spectrum modeling results for the newly
discovered luminous blue variable (LBV) in the NGC 1156 galaxy. Extended
atmosphere models were calculated using the non-LTE code CMFGEN. We have
obtained the luminosity of the discovered LBV $L\simeq (1.6\pm0.2) \times
10^{6} L_{\odot}$, effective temperature $T_{\text{eff}}=7.9\pm0.4$ kK and
mass-loss rate $\dot{M}f^{-0.5}= (8.2\pm1.0) \times 10^{-4}
M_{\odot}\text{yr}^{-1}$. The hydrogen abundance in the wind is $\approx20\,$%
for the metallicity $Z=0.5 Z_{\odot}$ of the host galaxy.
