The galaxy appears to be a merging system, characterized by two distinct, roughly spherical components. The two components have a golden, mature stellar population. There is a significant amount of tidal distortion indicating that it is in the late stages of a major merger.

The overall shape of the merged system is somewhat irregular, deviating from a perfect elliptical form, with a possible plume or extended structure. It appears relatively smooth in texture, lacking the distinct spiral arms or patchy star-forming regions. The combined luminosity suggests it is a massive galaxy. Star formation activity appears suppressed.
