The galaxy presents a generally smooth, elliptical morphology. It is characterized by a centrally concentrated luminosity profile that gradually fades outwards. The galaxy is nearly circular in appearance, exhibiting a minor axis ratio close to unity, suggesting a minimal degree of flattening. No distinct spiral arm structures or prominent dust lanes are discernible, supporting the classification as an elliptical galaxy. The overall color profile appears relatively uniform, with a slight bluish tint. The galaxy shows no signs of a major ongoing merger, only a very slight disturbance.
