The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall color is yellowish-orange, suggesting an older stellar population with fewer young, blue stars. The galaxy exhibits a high degree of circularity and does not show any obvious signs of spiral arm structure or a disk component. There is no clear indication of recent or ongoing major merger activity. The galaxy may exhibit a moderate amount of star formation, which would contribute to the intermediate color, but overall it appears to be a largely quiescent system.
