The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a substantial stellar population density. Moving outward from the core, the light gradually diminishes, indicating a decrease in stellar density. The overall color profile is dominated by redder hues, especially toward the center. The slight asymmetry in the shape is likely due to its late stage in the merging process, where the morphology appears to be slightly disturbed. It does not exhibit prominent spiral arms or distinct dust lanes. The smooth appearance suggests a more evolved system, potentially with a relatively low star formation rate. 
