The galaxy appears as a concentrated, yellowish-orange elliptical system. Its morphology exhibits a high degree of smoothness, lacking any discernible spiral arm structures or distinct features. The galaxy presents a somewhat circular shape, with a slight tendency toward elongation. There is no evidence of a recent major merger event. However, it is possible there has been a minor disturbance due to the slight distortion of the galaxy's overall shape. The color suggests an older stellar population, and suppressed star formation activity. The intense brightness is indicative of a large, relatively massive system. 
