The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. The light profile appears fairly uniform, with no discernible spiral arm structure. The galaxy exhibits a yellowish hue, suggesting an older stellar population with fewer hot, young stars. There appears to be only minor disturbance, and no visible signs of any ongoing major mergers. The galaxy appears relatively undisturbed and relaxed. Based on its color and morphology, this object is likely a massive galaxy with a relatively low star formation rate.
