The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The galaxy presents with a centrally concentrated luminosity profile, suggesting a high degree of central mass concentration. The color gradient indicates that the core is redder. The galaxy does not appear to display any prominent spiral arm structures or significant dust lanes. There is no evidence of a recent major merger event. The galaxy's light appears to be relatively uniform and symmetrical, further supporting the classification as an elliptical galaxy. The overall color suggests an older stellar population.
