The galaxy presents as a somewhat elliptical structure, appearing mostly smooth. A slight disclike structure can be observed. The central region exhibits a higher concentration of light intensity, indicative of a bulge component and/or active galactic nucleus. There is no apparent spiral arm structure within the visible spectrum. Coloration appears redder with low star formation. The galaxy is relatively large and massive. It is likely a mature galaxy. There is no evidence of any major disturbances that may be caused by a merger, however there are minor disturbances. It has an intermediate concentration of matter.