The galaxy presents as a relatively smooth, elliptical-like structure. It is highly concentrated in the center, with the light intensity gradually decreasing outwards, suggesting a high degree of central mass concentration. The color appears to be a blend of yellow and white, hinting at an older stellar population dominating the galaxy's composition, with a relatively quiescent star formation rate. There is a slight bluish hue in the outer regions which may indicate some younger stars, however it is not enough to classify this as a spiral galaxy. The galaxy exhibits a generally undisturbed morphology, showing no obvious signs of ongoing major mergers or tidal distortions. Its overall appearance suggests an evolved galaxy that has largely settled into a stable configuration.
