The galaxy displays a complex morphology, appearing as a multi-component system. One component is a bright, relatively smooth, and rounded central object exhibiting a bluish-white hue. This suggests a concentration of younger, hotter stars within this region. Another distinct component is visible as a diffuse, less concentrated structure offset from the brighter central object. This secondary component exhibits a yellowish-orange color, possibly indicative of an older stellar population or dust obscuration. Additionally, there seems to be some indication of a third, even fainter component, adding to the complexity of this galactic system. The presence of these separate, interacting components hints at ongoing or past gravitational interactions, potentially a merger event in progress or a tidal disturbance. The overall structure indicates a system that is not fully relaxed and potentially undergoing morphological transformation.
