The galaxy presents as a system with multiple distinct nuclei, potentially indicative of an ongoing or recent merger event. The dominant morphology appears to be elliptical or spheroidal in nature, although some features might be obscured by the merger activity. The central region exhibits a yellowish-white hue, which might suggest an older stellar population. A less pronounced redder area is visible, possibly indicating a region with more dust obscuration or older stars. There is also an area of bluish-white color, perhaps indicating a region with more active star formation. Overall, the galaxy displays a moderate degree of internal complexity, suggesting a system undergoing dynamic processes.
