The galaxy presents a largely smooth, elliptical morphology. It appears relatively undisturbed, showing no signs of ongoing major mergers or significant tidal distortions. The light distribution is concentrated towards the center, exhibiting a clear bulge component with a gradually fading halo. The color gradients suggest a radial change in stellar populations, with the core displaying a redder hue, possibly indicating older, more evolved stars. Moving outwards, the halo appears slightly bluer, suggesting the presence of a younger stellar population or lower metallicity stars. There is a very weak indication of a disk structure within the galaxy, or possible minor disturbances. The general appearance is that of a massive galaxy with a relatively low star formation rate.
