This galaxy appears to be a merging system, possibly in its late stages. It exhibits a generally smooth morphology with some disturbances present. The galaxy appears to have a primarily elliptical or spheroidal shape, showing only hints of a disk-like structure. The core regions are very bright and possibly contain active galactic nuclei. There is evidence of tidal interactions or minor disturbances in the surrounding regions. There may be ongoing star formation, though it is not dominating the light of the galaxy. Overall, the galaxy likely has a high mass and is exhibiting a low specific star formation rate. The system is moderately red, indicating the presence of an older stellar population.
