The galaxy appears to be in a late-stage merging process, exhibiting a disturbed morphology. The structure is elongated and somewhat irregular, suggesting gravitational interactions are actively reshaping its form. Two distinct, brighter regions are visible, possibly representing the remnant cores of the progenitor galaxies. The overall color is yellowish-red, suggestive of an older stellar population, although some bluer regions are present. There are no well-defined spiral arms or a central bulge, supporting its classification as undergoing a major interaction. The galaxy shows signs of significant tidal forces, implying a complex merger history. The star formation rate appears to be relatively low, based on the color index, which might be a consequence of the merger activity.
