(J004621.08+421308.2)

A status of a late A-type warm hypergiant has been assigned to this object based on the lack of detected He I emission [143]. In contrast to this, He I emission lines were reported by Sholukhova et al. [139], and an effective temperature of 10,000 K has been estimated from the modeling of the stars' spectral energy distribution [142]. The position of the object in the near-IR and WISE diagrams coincides with the B[e]SG domain.
