The galaxy presents a morphology consistent with a system undergoing a merger. Two distinct luminous regions are observed, connected by a fainter bridge of stellar material. The color gradients suggest differential stellar populations within the interacting components. One region appears more yellow/red suggesting an older stellar population. The other region shows blue/white colors possibly indicating ongoing star formation activity. The overall shape deviates significantly from a regular elliptical or spiral form, exhibiting an irregular, disturbed structure, which supports the merger classification. There is evidence of tidal features surrounding the main bodies, adding further credence to the ongoing interaction.
