The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a round morphology, appearing largely undisturbed. The color profile suggests a primarily older stellar population, emitting predominantly in the redder wavelengths. There is a slight indication of bluer light in the galaxy’s outer regions, although it's relatively subdued. There may be faint signs of disturbances within the galaxy. The galaxy possesses a substantial mass, and exhibits a modest amount of star formation.
