The galaxy presents as a generally smooth, elongated structure with a high degree of central concentration. The light distribution suggests an elliptical morphology. There is a clear color gradient across the galaxy, transitioning from a more yellowish-white core region to fainter, redder extensions. The dominant color indicates a stellar population that is primarily older, and less actively forming stars. The overall appearance lacks evidence of spiral arms or significant dust lanes, further supporting the classification as an elliptical galaxy. There is a hint of disruption or tidal features on one side, indicating possible past interactions.