This galaxy appears to be in a late stage of a merger. It exhibits a disturbed morphology with two distinct, bright nuclei embedded within a diffuse envelope of stars. The overall shape is somewhat irregular, lacking clear spiral arms or a well-defined disk structure. The galaxy's color is predominantly yellow-red, suggesting an older stellar population and reduced levels of ongoing star formation. There is a slight amount of bluer star formation in some areas, though this is not a dominant characteristic. The galaxy appears relatively smooth, with no distinct dust lanes or prominent HII regions visible. The overall light distribution is concentrated around the two nuclei, hinting at the remnants of two previously distinct galaxies now coalescing. Faint tidal features, possibly stellar streams, might be present at the very edges of the galaxy, though this is difficult to determine with certainty.
