This new variable star has gradually brightened. The object reached 12.34mag on 2001 October 3 from about 13.4mag on 2000 October (vsnet-campaign-unknown 1). S. Yoshida reported the gradual brightening has already started in 2000 October when the object was faint reaching 13.50mag (vsnet-campaign-unknown 2). T. Kato commented that if the object is a pre-main sequence emission-line star, the star may be an object belonging to a small subclass with occasional fadings like WW Vul, BO Cep etc (vsnet-campaign-unknown 3).