The galaxy appears to be undergoing a significant merger. Two distinct luminous cores are visible, suggesting the presence of two progenitor galaxies in the process of coalescing. The overall morphology is disturbed, with a diffuse halo of light extending beyond the main bodies. The color gradient suggests that the galaxy is comprised of both young blue stars as well as older redder populations. The presence of disturbed features implies elevated star formation, though the morphology is complex and dominated by the ongoing interaction. Based on the apparent luminosity, this appears to be a massive system. The generally elliptical shape suggests that it may eventually evolve into an elliptical galaxy as the merger completes.
