The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge with a diffuse halo. There is little indication of spiral arm structure or significant dust lanes within the visible light spectrum. The galaxy appears fairly round, with a very slight elongation. There is no strong evidence of any major mergers or tidal disturbances within the immediate vicinity of the galaxy. The galaxy's color is yellowish/white, suggesting a population of older stars. The galaxy seems to be a fairly passive system, with a low rate of star formation.
