The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light is dominated by older stellar populations, indicated by the overall yellowish-orange hue. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a high degree of central symmetry and roundness, with no obvious signs of recent major mergers or tidal disturbances. A faint, diffuse halo may be present, extending beyond the main body of the galaxy. The object appears generally relaxed and quiescent.
