The galaxy appears to be undergoing a significant interaction or merger event. There's a dominant, rounded component with a strong central concentration of light exhibiting a yellow-orange hue. This likely indicates an older stellar population within the core or bulge. Emanating from this central region are fainter, more diffuse structures exhibiting a bluer color. These structures appear to be tidal tails or debris, suggesting a disruptive gravitational influence. The shape of the galaxy as a whole deviates significantly from a smooth elliptical or spiral form, showing instead a complex, disturbed morphology. Dust lanes may be present within the more diffuse regions, contributing to the mottled appearance. The overall light profile appears to be relatively compact.
