Comparison of the Chandra X-ray image with the location of the outflow. This figure highlights a ∼10 X-ray count excess over the local azimuthal (background plus PSF wing) average, arranged in a semicircular arc ∼2″SW of the nucleus. The feature is labeled with a white arrow in the left panel, which shows the exposure-corrected Chandra/HRC image at the native pixel scale (013 per pixel). While the significance of < 2σ of this feature is too low for confident detection, it is co-spatial with the rim of the multi-phase outflow discussed in this paper. This is highlighted comparing the red (identical, WCS-matched) circles in both the Chandra and MUSE gas velocity dispersion panels (right and left, respectively).