  We report the identification of the bright (V${\sim}13.3$ mag) star FY Sct as
a long period detached eclipsing binary using a combined ASAS-SN and ASAS light
curve spanning 2000-2018. The orbital period is P${\sim}2.57$ years and the
primary eclipse lasts ${\sim}73$ days. The eclipse profile is suggestive of a
disk eclipsing binary rather than a stellar component. We also detect
${\sim}0.4$ mag pulsations with a period of P${\sim78}$ d. The next eclipse
begins on September, 28, 2018. Further photometric and spectroscopic
observations are encouraged, particularly when the system is in eclipse.
