The galaxy appears to be an elliptical galaxy with a smooth profile and concentrated light distribution, generally round in shape. There is some evidence of minor disturbances in its morphology. There is a brighter, more prominent object possibly indicating a core or central bulge. The overall color is indicative of an older stellar population, with a higher proportion of redder stars and a low rate of on-going star formation, though there does appear to be at least one area that could suggest on-going star formation or be another object within or interacting with the galaxy. There are also some indications of it possibly merging.
