Broadband SED from 2014 July 21 (MJD 56859.97) where a two-zone SSC model has been used to describe the overall emission. One emitting region is responsible for the gamma-ray, X-ray and partially optical emission (dashed blue line). A second component explains the radio emission together with some optical emission (dashed green line). The colored spectral points represent the data sample from 56859.97. The gray spectral points represent the archival spectral points taken from the SED builder at SSDC. The peak emission at ∼10¹⁴−10¹⁵ Hz is due to the host galaxy contribution, which is not taken into account in our SSC model of the jet emission.