The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The core region exhibits a high surface brightness, appearing bright and concentrated. The outer regions fade gradually, showing no distinct spiral arm structures or prominent dust lanes. The overall color is yellowish-white, possibly indicating an older stellar population dominating the light emission. There appears to be a slight flattening, suggesting it may not be perfectly spherical. There are no obvious signs of active star formation regions from the image alone. The general shape and luminosity profile suggest a relatively evolved system. Based on the disturbance levels, there may be slight tidal effects, or a very distant merging event.