The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. Two distinct nuclei are visible, one with a bluer color profile, and the other with a more reddish hue. The overall structure appears disturbed, with a complex, irregular shape. There is a dominant smooth component, but with visible indications of tidal features. The galaxy appears moderately bright, showing evidence of moderate star formation activity. The size appears to be of an extended but not extremely large object. The apparent roundness and lack of a distinct disk structure further support the likelihood of an elliptical or merging system morphology.
