The galaxy presents an elliptical morphology, appearing as a smooth, concentrated spheroid of light. The central region exhibits a bright, yellowish core, suggesting a significant population of older stars. Moving outward from the core, the light gradually diminishes, with a slight flattening apparent along one axis. This indicates a possible degree of rotational support or triaxiality. There is a subtle color gradient from the core to the outer regions, becoming slightly redder, possibly reflecting a change in stellar populations or dust content. No distinct features such as spiral arms, bars, or prominent dust lanes are discernible. The overall structure suggests a galaxy in a relatively evolved state, with a likely low rate of ongoing star formation. No signs of recent major mergers are apparent, although there is a small possibility of tidal interactions affecting the shape. The galaxy appears relatively isolated in the image field.
