> The superhump profile shows no signs of a double-waved pattern, and I could
> not detect early superhumps in my data. Yet, the large outburst amplitude of
> ~7.4 mag, and the long time for superhumps to develop (approx. 9 days) make
> this a very likely WZ Sge-type dwarf nova.
It would be worth noting that the period 0.065 d is
long for a WZ Sge star. If this is indeed a WZ Sge star,
it must be a period bouncer. Period bouncers tend to have
smaller amplitudes of ordinary superhumps and 0.14 mag
seems to be a bit large. I would propose to assign
the WZ Sge classification after confirmation of
a small Pdot and/or rebrightenings.