The galaxy presents as a merging system, with two distinct, relatively smooth components. The primary component appears roughly elliptical, displaying a yellowish-red hue suggesting an older stellar population with limited ongoing star formation. The second component is also smooth, similar in color, but smaller and slightly more defined than the primary object. Both components are undergoing significant tidal disturbances, including apparent distortions in shape. Overall, it seems to have a substantial mass with a relatively low star formation rate. The system is currently undergoing a merger of two distinct galaxies.
