We describe the optical spectrum of Wolf-Rayet star HD 4004 (WN 4b) in the
wavelength range from 3900 to 7000 Angstrom. Present observations reveal th
e stratification effects in the envelope of this star. Also evidence for va
riability of HeII line lambda 5411 is presented. Since no radial velocity v
ariations are observed in the optical spectrum of this star we conclude tha
t HD 4004 is a single Wolf-Rayet star and the observed emission line profil
e changes are of intrinsic nature.