uv-radial distributions of the Band 3 ACA (left) and ALMA (right) observations in which the visibilities are phase-shifted to the center of the SZ decrement. The colored lines show the median primary beam-attenuated elliptical SZ models based on the empirical formalism which are reported in Table 1. The shaded regions indicate the standard deviation in the uv-radial bin of the model and are thus a direct consequence of the eccentricity of the cluster. To gauge the uncertainty, we show the 0.16–0.84 quantiles of the mean A10-cc profile with the gray dash-dotted lines. The divergence of the A10-CC profile from the rest of the models and the introduction of eccentricity to the modeling of the SZ signal shows that the data disfavors a local cool core cluster as the morphological state of XLSSC 122. Other classifications cannot be separated because of the limited capabilities of ALMA+ACA in constraining fluxes at scales larger than about $2\stackrel{\prime }{.}0$ (∼1 kλ).