We have finished tonight observation on V4641 Sgr at Ouda. The obtained light curve is still calm, no short-term modulations are seen. In the light curve on May 29, there is gradual brightening trend during our run. This brightening seems to be explained with the normal elliptical modulations (due to the orbital motion of the secondary star), which have been observed at the quiescent state of V4641 Sgr. However, it might be a brightening to a new activity, so confirmation and follow-up time-series observations are encouraged. Regards, Makoto Uemura