The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a high degree of central concentration, appearing bright and somewhat diffuse. There is no distinct spiral arm structure visible. The galaxy's shape appears somewhat elongated, displaying an intermediate axis ratio. Faint color gradients are discernible, with the central regions potentially exhibiting a bluer hue compared to the outer areas. However, these color differences are subtle. No signs of major tidal disturbances or recent merger activity are readily apparent. The outer regions fade gradually into the background sky, lacking sharp boundaries or truncation.
