The galaxy appears to be in the process of merging or interacting with at least one other galactic structure. There is a primary, somewhat diffuse, central body that exhibits a mostly smooth morphology, with hints of some internal structure but lacking distinct spiral arms. Its color appears generally yellowish-white.

There is a distinct secondary condensation of light nearby that is whiter and more compact. These two bodies are likely gravitationally interacting. Further signs of interaction and/or possible tidal disturbances are hinted at, as well as the presence of star forming regions, indicated by reddish regions of star formation, and bluer regions that could be attributed to young stars.

Overall, the system seems to be a complex merging system. Further spectral analysis is needed to quantify the composition, star formation rates, and kinematics of the interacting components to better understand the dynamics of the merger.
