Gaia DR3 2893005857946801152 = ASASSN-23dr: most likely WZ Sge star
Berto Monard and Josch Hambsch have reported observations.
Using Monard's data, there appears to be a period of
0.05452(5) d with a double-peaked profile.
The result, however, is preliminary since the amplitude
was small (0.03 mag) and observations are still limited.
I used the name Gaia DR3 2893005857946801152 since this object
was selected as a variable by Gaia (there was probably
simply no concept of a dwarf nova in quiescence and was
classified as a WD). Please feel free to use ASASSN-23dr since
it is much shorter.