This galaxy presents as a somewhat elongated, though predominantly smooth object. Its structure exhibits characteristics somewhere between elliptical and disk-like morphology. It has some features that might indicate a disk but this is hard to verify. The light profile seems largely spheroidal and centrally concentrated. Color gradients are subtle, with a possible trend towards bluer colors in the outer regions of the galaxy. There does not appear to be any presence of strong spiral arms or a central bar. Indications suggest that the galaxy is not currently undergoing major merger events. The general smoothness suggests a lack of significant recent star formation, implying a relatively older stellar population.
