The galaxy presents as a predominantly elliptical or lenticular system, exhibiting a smooth, centralized luminosity profile with a high degree of spheroidal symmetry. A concentrated, bright core is evident, with a noticeable gradient in luminosity outwards, transitioning into a more diffuse halo. The primary color observed is redder in the center, with the outskirts of the galaxy exhibiting a slightly bluer hue, suggesting potential variations in stellar populations. There is no apparent disk or spiral arm structure, implying a lack of significant ongoing star formation activity. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.
