I present the interpretation of two consecutive M and C-class flares occurred on the solar disk on 2015 January 28 during 04:00 UT to 06:00 UT in NOAA AR 12268 using the ground based ARIES H-alpha and the space borne multi-wavelength data. The active region was highly complex and produced large number of M and C-class flares during it's span on the solar disk. Active region consists of two filaments F1 and F2 and only one filament F1 erupts resulting the failed filament eruption. The eruption speed of the filament F1 is around 20 kms-1 and the falling speed is about 60 kms-1. Other filament F2 is not associated to any flare as there was no energy build up due to the small scale magnetic field. Although the flare occurred with F1 was highly energetic and reaches to the umbra of the active region. The filament eruption fails due to the high-lying magnetic field lines extrapolated using PFSS.