I report the discovery of a prominent broad and asymmetrical feature near 6.4 keV in the Seyfert 1 MCG-02-14-009 ( z=0.028 ) with XMM-Newton /EPIC .
The present short X-ray observation ( PN net exposure time \sim 5 ks ) is the first one above 2 keV for MCG-02-14-009 .
The feature can be explained by either a relativistic iron line around either a Schwarzschild ( non-rotating ) or a Kerr ( rotating ) black hole .
If the feature is a relativistic iron line around a Schwarzschild black hole , the line energy is 6.51 ^ { +0.21 } _ { -0.12 } keV with an equivalent width of 631 ^ { +259 } _ { -243 } eV and that the inclination angle of the accretion disc should be less than 43 ^ { \circ } .
A relativistically blurred photoionized disc model gives a very good spectral fit over the broad band 0.2–12 keV energy range .
The spectrum is reflection dominated and this would indicate that the primary source in MCG-02-14-009 is located very close to the black hole , where gravitational light bending effect is important ( about 3–4 R _ { g } ) , and that the black hole may rapidly rotate .