V4744 Sgr further spectrum by Fujii Mitsugu Fujii (Fujii Bisei Observatory, Okayama, Japan) obtained the following spectrum on Nov. 4. http://vsnet1.harenet.ne.jp/~aikow/v4744sgr_20021104.gif The spectrum shows stronger H-alpha (FWHM 950 km/s) and H-beta emission lines, stronger P Cyg-type profile of the Na D line. The spectrum clearly shows Fe II series emission, indicating that the object is most likely an Fe II-class nova caught in an early stage of its evolution.