The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-orange hue, potentially indicating an older stellar population with a lower rate of star formation. The galaxy is largely spheroidal in shape. There is little indication of spiral arms or significant dust lanes. Subtle indications suggest it is not perfectly spherical, but rather somewhat elliptical. There is no strong evidence of recent or ongoing major merger events.
