The galaxy presents a relatively smooth, elliptical morphology. It appears nearly spherical. The color profile suggests a relatively evolved stellar population, with a redder hue indicative of older stars dominating the light output. There may be some ongoing star formation or recent interactions as the galaxy's light is not entirely uniform. There seems to be no discernible dust lane or spiral arm structure within the galaxy. Some level of disturbance can't be ruled out, but the object generally appears relaxed.
