This galaxy appears to be a relatively smooth, elliptical galaxy with a dominant central bulge. The galaxy exhibits a somewhat elongated shape, deviating slightly from perfect circularity. It possesses a yellowish hue overall, indicative of an older stellar population and lower rates of current star formation. There is a subtle hint of some kind of disturbance in the galaxy shape, though not indicative of a major merger event. The core is very luminous, but relatively small in radius. 
