The galaxy presents as a centrally concentrated object with a smooth appearance. Its overall shape is elliptical, appearing mostly round. A faint, diffuse halo surrounds a brighter, more compact core. The color gradient suggests an aging stellar population, with the central region exhibiting a redder hue possibly indicative of older stars or dust obscuration. There is no apparent spiral structure, and the galaxy does not appear to be undergoing any major mergers or tidal disturbances. Faint, subtle color variations are visible within the halo, which might suggest subtle variations in stellar population or composition.
