The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-orange hue, possibly indicating an older stellar population with fewer young, hot, blue stars. The overall shape is quite round with very little discernible disk-like structure. No signs of major mergers or significant tidal disturbances are visible. There is a slight elongation, but this is minor. The light is centrally concentrated, with a rapid falloff in surface brightness moving outwards from the core. There may be a very faint, extended halo. Star formation appears to be low.
