The galaxy appears to be relatively smooth and elliptical in shape, with a high degree of roundness. There seems to be evidence of a potential merger, likely in progress. There is a large central concentration of light suggesting a dominant bulge component. There appears to be a smaller concentration of light nearby, which could be either a smaller galaxy that is merging or simply a concentrated region of star formation within the larger galaxy. There is also a very faint and small concentration of light a bit farther away that could be a much smaller companion galaxy. The galaxy exhibits a fairly uniform color profile across its extent, which suggests a relatively old stellar population throughout. There may be signs of a minor tidal disturbance or asymmetry in the outer regions.
