The galaxy appears to be undergoing a significant merger event. The main body is a relatively smooth, centrally concentrated object, suggestive of an elliptical galaxy or the bulge component of a spiral. However, there's clear evidence of disturbance in its morphology. There is a brighter region and a less bright region. These components are connected, but not fully coalesced. The system displays an irregular shape with light distribution showing significant deviations from a perfect elliptical or spiral structure. The galaxy shows a bluer tint in some regions, hinting at some active star formation. Overall, this appears to be a galaxy at an interesting stage of evolution, likely transitioning towards a more relaxed and uniform structure.
