The galaxy appears as an elliptical morphology, with a smooth, centralized light distribution. The core region exhibits a bright, concentrated luminosity, indicating a potential bulge component. The isophotes appear relatively regular, suggesting a well-mixed stellar population. There is no distinct spiral arm structure or dust lane visible. It shows a slight elongation, but it is predominantly round. Faint, extended light is observed beyond the brighter central region, suggestive of a diffuse stellar halo. The overall color appears somewhat blue-white. The image does not indicate any major disturbances, such as tidal tails or obvious signs of ongoing mergers. There may be subtle features indicating a minor disturbance but this is not fully visible in the image. 
