In this work , we continue the study of the central region of NGC 613 by \citet paty , by analysing the stellar and gas kinematics and the stellar archaeology in optical and near-infrared data cubes .
The high spatial resolution of the Gemini Multi-Object Spectrograph ( GMOS ) data cube allowed the detection , using spectral synthesis methods , of an inner circumnuclear ring , with a radius of \sim 1 arcsec , composed of \sim 10 ^ { 9 } -yr stellar populations .
Such a ring is located between the nucleus and the circumnuclear ring composed by H ii regions detected in previous works .
Besides that , there is a stellar rotation around the nucleus and the rings follow the same direction of rotation with different velocities .
The intensity-weighted average stellar velocity dispersion at the centre is 92 \pm 3 km s ^ { -1 } .
Three distinct gas outflow components were detected .
The direction of the outflow observed with the H \alpha emission line is compatible with the direction of the previously observed radio jet .
The direction of one of the outflows detected in the [ O iii ] \lambda 5007 emission coincides with the axis of the ionization cone .
There is no difference regarding the stellar populations and the stellar kinematics along the double stellar emission , probably separated by a dust lane as mentioned in Paper I , confirming that they are part of the same structure .