Unfiltered time-series runs, made on seven consecutive nights from 2019 Sept. 29.8 UT (JD = 2458756.3), did not reveal any periodic variation with an amplitude > 0.02 magnitudes down to 50 cycles/day (2019ATel13180...1L). Subsequently, superhumps with an amplitude of 0.28 mag and a period of 0.057(2) d were detected 2019 Oct. 17–21 (vsnet-alert 23650, 2019ATel13225....1L). Spectroscopy on 2019 Oct. 12 revealed strong, narrow H-alpha emission on top of broader H-alpha absorption and Balmer absorption lines, consistent with that of a dwarf nova in outburst (J. Rupert, TNS). The epoch is for the optical peak of the 2019 superoutburst.
Type from vsnet-alert 23650, 2019ATel13225....1L, and vsnet-alert 23657. Position based on astrometry by T. Vanmunster (personal communication). "Eruption" year deleted.