  I analyzed All-Sky Automated Survey for Supernovae (ASAS-SN) Sky Patrol data
of ES Dra and classified it to be a Z Cam star with VY Scl-type fading
episodes. An analysis of Transiting Exoplanet Survey Satellite (TESS)
observations showed that this object shows shallow eclipses and that the
orbital period is 0.17749895(17) d. Negative superhumps with a period of
0.167830(2) d and the beat phenomenon between the period of negative superhumps
and the orbital period were detected in the TESS data between 2020 January and
March. The orbital profile systematically varied depending on the beat phase
and eclipses were missing in some phases. The eclipses in ES Dra were grazing
and the disk was probably not eclipsed in some phases depending on the
orientation of the tilted disk. These observations added a support to the
interpretation of the precessing, tilted disk as the origin of negative
superhumps. Negative superhumps disappeared 4 d before the VY Scl-type fading
started. It was likely that the mass-transfer rate quickly dropped when
negative superhumps disappeared and the decline of the total luminosity of the
disk took 4 d. This provides a measurement of the time-scale of the response of
the disk against a sudden decrease of the mass transfer in a VY Scl star.
Although one of standstills in ES Dra was terminated by brightening, the
identity of ES Dra as an IW And star would require further events.
