The galaxy presents a largely smooth, centrally concentrated morphology. It has a softly luminous core, and overall appears to be of an elliptical or lenticular type. The light profile fades gradually outwards from the center with a fairly uniform color gradient and a small amount of distortion in its overall shape. No distinct spiral arms or bar structures are readily apparent. The galaxy's light appears to skew to the redder side of the spectrum, but it is still quite bright. There may be only the faintest hint of a disk in the image. The mass appears substantial.
