The galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of central concentration with a bright, well-defined core that is orange in color, suggesting a population of older stars. A yellow-greenish halo surrounds the core, gradually fading into the background. The galaxy appears quite round with no obvious signs of spiral arms, bars, or significant disturbances. Its overall morphology points towards a lack of active star formation and minimal evidence of recent or ongoing mergers. The galaxy's appearance is consistent with a massive early-type galaxy at a considerable distance.
