The galaxy presents as a smooth, elliptical-like structure. There is a concentrated central bulge that appears bright and has a yellowish hue, suggesting an older stellar population. Moving outward from the center, the light gradually diffuses into a fainter halo. There is a hint of a disk-like structure, however, it is faint and lacks any well-defined spiral arms or prominent dust lanes. The overall appearance is relatively undisturbed, exhibiting no signs of major mergers or significant tidal distortions, indicating a gravitationally settled state. The light distribution suggests a high degree of central concentration.
