The galaxy appears to be in the late stages of a major merger, exhibiting a disturbed morphology. Two distinct nuclei are visible, each with a relatively smooth, rounded appearance. The nuclei are separated by what appears to be a bridge of diffuse stellar material. The overall color of the galaxy is yellowish-white, suggesting an older stellar population, although some hints of bluer regions are present, potentially indicating pockets of recent star formation. The galaxy seems to be relatively compact, with a defined edge. Tidal tails or other extended features characteristic of mergers are not immediately obvious, indicating that these features may be faint or obscured.
