ES Dra: UGZ+VY Scl ASAS-SN data: https://asas-sn.osu.edu/light_curves/1518b1b9-29d1-4803-b653-0e4330e6e395 Recent twi fadings (2019 Aug. and 2020 Apr.) were long (lasting a month) and showed slow recovery. This cannot be explained by Z Cam-type quiescence and is better interpreted by mass-transfer variation, i.e. VY Scl-type phenomenon.