Superhumps in SU UMa CCD time-series photometry on Jan. 9 (Ouda team rooftop station, 25-cm SCT + ST-7 unfiltered) has revealed the presence of large-amplitude superhumps (exceeding 0.4 mag). The best superhump period determined using the PDM method was 0.0780 d, superhump maxima ocurring on 9.467, 9.549, 9.631 UT etc. The present observation has confirmed that the superoutburst, in addition to the immediate precursor on Jan. 7, was preceded by a photometrically unusual normal outburst, exhibiting transient superhump activity. Regards, Taichi Kato