Two-dimensional maps of integrated light, stellar velocity, and stellar velocity dispersion. Left panel: map of integrated light within the MUSE spectral range. The isophotes are shown as contours of 50%, 10%, 5%, 1%, and 0.5% of the peak flux value. Regions with lower flux were masked out of the image. Middle panel: line of sight stellar velocity. Right panel: stellar velocity dispersion. North is up, east is left, the origin is defined as the position of the AGN, and 10 arcsec corresponds to 2.2 kpc. The point source south of the nucleus is a foreground star that was masked out in the centre and right panels.