Stellar mass surface density map of the center of NGC 2300 group obtained by combining Spitzer’s IRAC 1 and IRAC 2 images using stellar mass relation from Querejeta et al. (2015). Red cross shows the group X-ray IGM emission center from Mulchaey et al. (1993). LOFAR contours of the radio continuum emission (Roberts et al. 2024) at 144 MHz (3, 6, 12, 24, 48, 96, 192–RMS, RMS = 60 μJy, and resolution = 4.9 × 4.3 arcsec²) shown overplotted in white. Golden arrow shows the predicted trajectory of NGC 2276, derived from the direction of the radio continuum tail (Souchereau et al. 2025), along with the Hα kinematics (Haan & Braun 2014).