Top: Spitzer Space Telescope images of SNhunt120 obtained on +28 d, +39 d, and +1155 d at 3.6 μm and 4.2 μm, the position of the transient is indicated with a red circle. Bottom: two-panel plot containing SEDs constructed for SNhunt120 at early and late phases, along with BB fits. The early SED is constructed with CSP-II photometry taken on +36.8 d and Spitzer measurements obtained by interpolating between estimated magnitudes obtained from +28 d and +39 d images. A BB function fit (blue dashed line) characterized by a temperature of K is overplotted on the early SED. The BB reproduces the fluxes from u to H band. However, the Spitzer MIR fluxes are clearly above the flux level of the best BB fit, suggesting the presence of an additional cooler component. The SED constructed using the +1155 d Spitzer flux points is fit with a BB function characterized by K.