The galaxy appears to be in the late stages of a merger. Two distinct nuclei are visible, one exhibiting a more reddish hue, potentially indicating an older stellar population or significant dust obscuration, and the other a yellowish tinge. The galaxy exhibits a generally smooth morphology overall, though there are some minor irregularities in the light distribution. The shape appears elongated, but not highly so, suggesting an evolution towards a more elliptical form as the merger progresses. There is no strong evidence of tidal tails or extended streams of stars.