The galaxy appears to be a relatively smooth, elliptical system. Its overall color is yellowish-white, suggesting an older stellar population with fewer young, hot stars. The galaxy exhibits a somewhat concentrated central region, with a gradual decrease in luminosity towards its outer edges. There is no obvious dust lane or spiral structure visible. A slight elongation is apparent, indicating a deviation from a perfectly circular shape. No signs of ongoing major merger activity are readily observable, though a minor disturbance cannot be entirely ruled out based solely on this image.
