The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, possibly indicating a lack of significant recent star formation. The galaxy exhibits a generally round morphology, with a slight elongation that indicates it is not perfectly spherical. No prominent spiral arms or distinct dust lanes are visible, supporting its classification as an elliptical galaxy. The outer regions fade gradually into the background sky, suggesting a diffuse halo. There is no obvious evidence of major merging or tidal disturbances in this image.
