Mitsugu Fujii (Okayama, Japan) obtained a low-resolution spectrum of the object on July 7.629. The spectrum shows Balmer series, Fe II (multiplet 37, 42, 48, 49, 55, 73, and 74), Na I D, O I(777.3, 844.6 nm), and Ca II (849.8, 854.2 nm) emission lines. These features indicate that the object is a Fe II-class nova.