We have performed reduction of images taken at last night at Ouda. The obtained light curve revealed that the object is still active, but amplitudes of short-term modulations are somewhat small. The most prominent feature is a large hump with an amplitude of 1 mag around May 26.66 UT. The light curve is similar to that observed on May 25, except for shorter-time scale oscillations are weak. The object has returned to its quiescent level, but time-series observations are still needed. Regards, Makoto Uemura