1. Introduction

2. Data
2.1. Observations and data reduction
2.2. Optical Imaging
2.3. IFU optical observations
2.4. Deblending the AGN and host emission

3. Analysis & Results
3.1. Fitting the stellar continuum and the ionized gas emission
3.2. Mapping the emission line properties
3.3. Kinematic modelling

4. Discussion
4.1. Star Formation as potential driver for the AGN fuelling
4.2. Chemical Enrichment of the CNE
4.3. On the black hole feeding mechanism

5. Summary and Conclusions