The galaxy presents as a fairly regular elliptical galaxy with a smooth morphology. The central bulge is bright and yellowish, suggesting an older stellar population dominated by redder giants. The isophotes appear generally round. There is a faint halo surrounding the central bulge, with a gradual decrease in surface brightness moving outwards. There are minimal signs of dust lanes or spiral arms in the galaxy. There is no apparent major disturbance or ongoing merger activity; it appears to be a relatively relaxed system.
