The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that is bright and yellow-white in color. Moving outwards from the core, there is a gradual decrease in luminosity, with the surrounding halo exhibiting a more diffuse and reddish-orange hue. The galaxy appears generally rounded, with no discernible spiral arm structures or significant dust lane features. There is no obvious major merger activity, but there is a hint of a minor disturbance in the halo region. Overall, this galaxy appears to be a massive, evolved system, likely with a low rate of star formation.
