The galaxy appears to be in the late stages of a merger. Two distinct nuclei are visible, connected by a stream of diffuse light, indicating tidal interactions. The overall morphology is highly disturbed, lacking clear spiral arms or a well-defined disk. The system presents a somewhat rounded, though irregular, shape.

The light is generally red, with a yellowish core and redder outer parts. Star formation appears low, given the lack of bright blue regions. A low star formation rate also suggests that most of the gas has already been used up. The system is relatively massive.
