The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a centrally concentrated luminosity profile. The core region appears a yellowish-white, suggesting an older stellar population. The galaxy has a relatively high degree of roundness, with minimal indication of a disk structure or spiral arms. There is no clear evidence of ongoing major mergers or significant tidal disturbances. A faint, diffuse halo or envelope surrounds the central region. Overall, this galaxy exhibits characteristics consistent with a massive, evolved system with a low star formation rate.
