The galaxy appears to be a somewhat irregular, disk-like structure with a noticeable central bulge. There's a hint of spiral arm structure or flocculent arms extending outwards. The galaxy exhibits a blueish hue overall, possibly indicating ongoing or recent star formation, particularly towards the center of the galaxy. The outer regions appear to be more diffuse, and difficult to discern due to image resolution. Overall, it is likely undergoing significant disturbances and perhaps a merger.
