The galaxy presents a largely smooth and elliptical morphology, displaying minimal evidence of spiral arm structures or significant disk features within the observed optical wavelengths. It appears concentrated and moderately luminous, exhibiting a radial color gradient shifting from a yellowish-white core region to a redder outer halo. The morphology suggests a galaxy that is not currently undergoing a major merger event. There are no obvious tidal tails or strong distortions in the shape of the galaxy; however, a minor disturbance cannot be ruled out. The relative lack of blue light and disk features indicates that star formation activity is subdued within the galaxy. The galaxy's roundness suggests it is viewed close to face-on, rather than edge-on.
