The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light profile. There is a subtle elongation observed, suggesting a deviation from perfect circularity. The galaxy's color gradient indicates a redder core, potentially indicative of an older stellar population. The outer regions appear bluer, potentially hinting at the presence of younger stars, though this is less pronounced. There is no prominent disk structure or spiral arms visible, nor are there any obvious signs of recent major merger activity. The galaxy does not show a well-defined nucleus, its central region is rather diffuse. 
