SU UMa superoutburst? CCD photometry on Jan. 8 (Ouda team rooftop station, 25-cm SCT + ST-7 unfiltered) revealed the presence of apparent superhumps superimposed on the gradually fading trend. The period is longer than 0.08 d, undoubtedly longer than the orbital period. Observations are strongly recommended in order to see whether the present outburst indeed turns into a super- outburst. The observation tonight looks like to show the object still bright. Regards, Taichi Kato