The galaxy appears to be in a state of advanced merging, with a notable disturbance to its overall morphology. The primary structure exhibits two distinct, luminous concentrations, likely representing the cores of the merging galaxies. These cores are bright, indicating a high density of stars and potentially active galactic nuclei. 

There is a generally smooth appearance to the central region, with a significant fraction of the light being emitted from older stellar populations. However, there are some indications of ongoing or recent star formation, represented by bluer hues interspersed throughout the main body. Redder regions may indicate areas of dust obscuration or older stellar populations.

Based on the apparent disturbance and merging activity, a considerable fraction of this galaxy's overall mass is likely concentrated in its center. The system is likely in the process of dynamically relaxing towards a final, more stable configuration, which might eventually lead to a single, more spheroidal system.
