The galaxy presents as a merging system, seemingly in the late stages of interaction. One core appears more diffuse and blue-shifted, possibly indicating ongoing star formation, while the other is more concentrated and has a redder color, suggestive of an older stellar population. The overall morphology is significantly disturbed; the galaxy shows little to no defined structure, with a bright central region dominated by the two interacting cores, and a more diffuse halo. The shape is elongated but distorted, with tidal features difficult to resolve due to distance.
