The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that emanates a yellowish-white light. The galaxy demonstrates a high degree of circular symmetry. No distinct spiral arms, bars, or other prominent features typically associated with disk galaxies are discernible. The outer regions of the galaxy fade into a diffuse halo, exhibiting a reddish hue. There is no indication of any major ongoing merger activity, though there is some slight indication of minor disturbances in its form. The color suggests it is composed of older, redder stars. Overall, the galaxy presents an appearance consistent with an evolved stellar population and reduced levels of star formation.
