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We present Australia Telescope Compact Array radio data of the dwarfirregular galaxy ESO 324-G024 which is seen in projection against the giant,northern lobe of the radio galaxy Centaurus A (Cen A, NGC 5128). The distortedmorphology and kinematics of ESO 324-G024, as observed in the 21 cm spectralline emission of neutral hydrogen, indicate disruptions by external forces. Weinvestigate whether tidal interactions and/or ram pressure stripping areresponsible for the formation of the HI tail stretching to the northeast of ESO324-G024 with the latter being most probable. Furthermore, we closely analyzethe sub-structure of Cen A's polarized radio lobes to ascertain whether ESO324-G024 is located in front, within or behind the northern lobe. Ourmulti-wavelength, multi-component approach allows us to determine that ESO324-G024 is most likely behind the northern radio lobe of Cen A. This resulthelps to constrain the orientation of the lobe, which is likely inclined to ourline of sight by approximately 60 degrees if NGC 5128 and ESO 324-G024 are atthe same distance.

Blasting away a dwarf galaxy: The "tail" of ESO 324-G024