R. Novak has kindly sent us data sets on December 23 and 24 during the superoutburst. Combined with his data, the data taken at Kyoto on December 22, 23, 24, 25, and 26 yields the best candidate of the superhump period of 0.078483 day, which is slightly shorter than the previous result. The average superhump light curve is a typical one for that of SU UMa star in superoutburst. The outburst have already been terminated, but colse monitorings for possible re-brightening are encouraged. Regards, Makoto Uemura