The light curve observed at Ouda on May 25.62-25.8 UT has revealed that the object is now slightly above the quiescent level, and still active. The light curve shows minutes-order fluctuations with amplitudes of 0.4mag, and furthermore, an 1-mag big hump during 25.69-25.72 UT. A possible another big hump can be seen during 25.76-25.78 UT although clouds heavily disturbed observations at that time. Hence, although the object apparently faded, the short-term modulations can still be seen. Follow-up observations are encouraged. Regards, Makoto Uemura