The galaxy presents as an elliptical form with a high degree of central concentration. There is a noticeable color gradient, transitioning from a bluer hue at the outer edges to a redder tone toward the nucleus. The observed ellipticity is significant, indicating a flattened shape. A faint halo or extended envelope of diffuse light is visible, surrounding the primary body of the galaxy. There appear to be no prominent spiral arms or significant dust lanes. Surface brightness appears relatively smooth and uniform across the galaxy, with no indications of intense star formation regions directly apparent in the available imagery. There are signs of an irregular halo around the galaxy, and a slight flattening, meaning the sersic index may be very low.
