Аннотация:We present the results of observations of the Irr galaxy IC 10 at the SAO RAS 6-m telescope with the SCORPIO focal reducer operating in the long-slit spectrograph mode. The work has been continued after the conference and here we add the new results of the integral-field MPFS observations of the galaxy. Based on these data we have analyzed the ionized-gas emission spectrum in the region of intense star formation and refined the gas metallicity estimates. Using the new improved ionization models by Martin-Manjon et al. [1], we have determined the gas ionization parameters and ionizing-clusters ages and masses from the spectra of the investigated HII regions. The cluster ages and masses are shown to be within the ranges 2.5–5 Myr and (0.2–1)×105M, respectively. We have determined the relative O/H, N/H and S/H abundances in about twenty HII regions of the galaxy.