The galaxy presents an elliptical morphology, appearing as a relatively smooth, featureless spheroid. The color profile suggests a somewhat older stellar population. It appears slightly flattened, with the major axis oriented in a roughly east-west direction. There is a subtle central concentration of light, though it does not appear intensely bright or indicative of a highly active galactic nucleus. The outer edges of the galaxy fade gradually, with no sharp truncation of the stellar distribution, leading to a diffuse, hazy appearance. There is a hint of substructure within the galaxy.