The galaxy presents as an elliptical morphology, although there is some slight asymettry, possibly indicating it may be transitioning from a spiral. It appears relatively smooth in texture. The central bulge is quite prominent, with the overall color suggesting an older stellar population, indicative of lower star formation. The galaxy displays a somewhat elongated shape; it is not perfectly circular. There is no clear evidence of a major ongoing merger, although some minor disturbances might be present in the form of slight distortions.
