The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a high degree of roundness. There is a central, luminous bulge that dominates the overall brightness of the galaxy. The galaxy exhibits a color gradient, appearing more yellow/orange in the central bulge. This suggests an older stellar population dominates the galaxy. Fainter, bluer regions can be seen extending away from the bulge. No prominent spiral arms or significant dust lanes are discernible in the image. There is no evidence of any major merger events or tidal disturbances. The galaxy appears to be a relatively undisturbed system.
