The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. Its overall shape is nearly circular, with a slight elongation evident. The light profile appears centrally concentrated with a gradual decline in intensity moving outward from the core. The core is bright and somewhat blue, suggesting a population of relatively young stars. The outer regions exhibit a redder hue, perhaps indicating an older stellar population. No obvious spiral arm structure or dust lanes are apparent, supporting its classification as an elliptical galaxy. There are no obvious signs of any major mergers or interactions.
