  Warps are vertical distortions of the stellar or gaseous disks of galaxies.
One of the proposed scenarios for the formation of warps involves tidal
interactions among galaxies. A recent study identified a stellar warp in the
outer regions of the south-western (SW) disk of the Large Magellanic Cloud
(LMC) and suggested that it might have originated due to the tidal interaction
between the LMC and the Small Magellanic Cloud (SMC). Due to the limited
spatial coverage of the data, the authors could not investigate the counterpart
of this warp in the north-eastern (NE) region, which is essential to
understanding the global shape, nature, and origin of the outer LMC warp. In
this work, we study the structure of the LMC disk using data on red clump stars
from the Gaia Early Data Release 3 (EDR3), which cover the entire Magellanic
system. We detected a warp in the NE outer LMC disk which is deviated from the
disk plane in the same direction as that of the SW outer warp, but with a lower
amplitude. This suggests that the outer LMC disk has an asymmetric stellar
warp, which is likely to be a U-shaped warp. Our result provides an
observational constraint to the theoretical models of the Magellanic system
aimed at improving the understanding the LMC-SMC interaction history.
