This galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent merger event. It presents an overall rounded shape, though with some deviation from perfect circularity. The light distribution is centrally concentrated, appearing smooth with a lack of clearly defined spiral arms or a prominent disk structure. There is an observed color gradient, shifting from bluer hues in some regions to redder colors in others, consistent with the possibility of varied stellar populations and star formation activity. The galaxy appears as a dual core structure with a degree of disturbance to the overall shape. It looks like it may be two galaxies coming together.
