  In this letter, motivated by double-peaked broad Balmer emission lines
probably related to tidal disruption events (TDEs), a potential TDE candidate
is reported in SDSS J160536+134838 (=SDSS J1605) at $z\sim0.44$ having
quasar-like spectrum but with double-peaked broad H$\beta$. The long-term CSS
light curve can be naturally described by a main-sequence star of
$2.82_{-0.19}^{+0.20}{\rm M_\odot}$ disrupted by the central black hole (BH) of
$144_{-21}^{+26}\times10^6{\rm M_\odot}$ in SDSS J1605. Meanwhile, the ASAS-SN
light curves afterwards show none apparent trend variability, indicating the
bright CSS flare in SDSS J1605 unique and different enough from variability of
normal AGN. Furthermore, there is a consistency between the TDE model
determined sizes of debris with the sizes of emission regions for the
double-peaked broad H$\beta$ described by the accretion disk model, supporting
the disk-like BLRs probably related to a central TDE in SDSS J1605. And the
virial BH mass $\sim$7 times higher than the TDE model determined value can be
naturally explained by R-L relation determined BLRs sizes very larger than the
actual distance of emission regions related to TDEs debris in SDSS J1605.
Although no clear conclusion on double-peaked broad lines absolutely related to
TDEs, the results here provide clues to detect potential TDEs in AGN with
double-peaked broad lines.
