The galaxy presents as a largely smooth, elliptical or spheroidal structure. It exhibits a concentrated, luminous core that fades into a more diffuse halo. The color profile appears consistent, with a yellowish hue dominating the overall appearance, suggesting an older stellar population and reduced active star formation. There is no discernible disk component or spiral arm structure visible. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Faint asymmetrical extensions may indicate minor tidal features, but these are subtle. Overall, the galaxy appears to be a passively evolving system.
