V838 Mon spectrum (Fujii) M. Fujii (Fujii Bisei Observatory) commnicates that he took 19 spectra within 7 hours on Feb. 3. A preliminary quick-look analysis has revealed the presence of strong H-alpha and H-beta emission (FWHM of H-alpha 12 A). There seems to be likely Fe II emission line series, accompanied with a P Cyg profile. The P Cyg profile was getting stronger with time. However, the continuum still resembled a K-type star. No striking brightening was observed in the short wavelength region.