Position of NGC 1272 (in red) on the M_BH − r_b (left), the M_BH − M_* (middle), and the M_BH − σ (right) relation. The black data points are from Rusli et al. (2013a), Saglia et al. (2016), Thomas et al. (2016), Mehrgan et al. (2019), Neureiter et al. (2023), and de Nicola et al. (2024). The blue data points are core ellipticals with a stellar mass of greater than 10¹² M_⊙. While the galaxy follows the M_BH − r_b given by Thomas et al. (2016) and the M_BH − M_* relation of Saglia et al. (2016) for the sample of CorePowerE, it deviates by a factor of 8.4 from the M_BH − σ relation of Saglia et al. (2016), or by a factor of 1.8 of the 1σ error combined with the intrinsic scatter in the relation (shown by the dotted lines).