The galaxy exhibits an apparent disturbed morphology, suggesting an ongoing or recent interaction with another galaxy. A significant portion of the Galaxy Zoo volunteers classified it as a merger. There are two distinct luminous regions. One of the regions exhibits a redder hue, possibly indicative of an older stellar population or higher dust content. The other region appears bluer, potentially suggesting a younger stellar population and active star formation.

There is evidence of faint tidal features extending away from the main body of the galaxy. The galaxy exhibits a notable disk-like component, although it is heavily disrupted. A notable feature is the presence of diffuse light surrounding the central regions, possibly indicating a stellar halo or tidal debris. The overall color of the galaxy is moderately blue-shifted, which places the galaxy at a significant cosmological distance.
