This galaxy presents an asymmetrical morphology. The primary luminous component appears relatively smooth and centrally concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. There is a secondary, less luminous component offset from the primary. It shows more reddish and yellowish colors, potentially indicative of either ongoing star formation or a dust-reddened stellar population. 

There is some evidence of faint tidal features or disturbances. The faint extensions emanate from the core that could be indicative of past or ongoing interactions with another galaxy. Based on its overall morphology, it's difficult to classify this as a pure elliptical or spiral galaxy. The presence of disturbances, the two core components, and the colors of the stellar population point toward a possible ongoing merger.
