The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. There is minimal visible disk structure, and the galaxy appears mostly spheroidal. The light profile suggests a fairly uniform distribution, with a possible slight elongation. Its color is predominantly yellow to red, indicating an older stellar population, but there is some green to bluish light also visible in the outer parts of the galaxy. There is no apparent sign of spiral arms, and the core is relatively compact and bright. There are very minor disturbances to the galaxy's morphology. The galaxy has likely undergone minimal merging events.
