The galaxy appears to be an interacting system, possibly in the late stages of a merger. Two distinct luminous cores are visible, with diffuse material extending between them. The overall shape is irregular and elongated, lacking a well-defined disk structure. The color is generally yellow-white, which may indicate an older stellar population and relatively low ongoing star formation. Some possible dust lane regions can be observed near the centers of the cores. Based on the apparent disturbed morphology, tidal tails or bridges might be expected, but the image resolution is insufficient to confirm their presence. The primary morphological classification appears to be a merging galaxy with a smooth component.
