The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal with a high degree of central concentration. The light distribution suggests a relatively old stellar population, with a significant red component. The lack of pronounced spiral arms or dust lanes indicates that star formation is low. There is a slight indication of a tidal tail feature extending upwards; if real, this could indicate a past or ongoing minor interaction with another galaxy. Overall the galaxy appears to be a fairly relaxed, undisturbed system.
