The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a concentrated, bright core that appears yellowish in color, suggesting an older stellar population dominates this area. The light gradually diffuses outwards from the core, forming a halo-like structure. There is only slight indication of a disk. No apparent spiral arm structures or significant dust lanes are observed within this galaxy. The overall structure is quite regular, with no major tidal disturbances or indications of ongoing mergers visible.
