The galaxy presents as a smooth, elliptical-like structure. It appears to exhibit a high degree of central concentration, with the light intensity gradually decreasing from the core outwards. The overall color is yellowish, suggesting an older stellar population, but also appears to have some bluer areas, implying the possibility of ongoing, though modest, star formation. There is no discernible disk or spiral arm structure. The galaxy seems relatively undisturbed, showing no clear evidence of major mergers or tidal interactions. Minor disturbances or minor mergers, though, cannot be fully excluded.
