The galaxy presents as a relatively smooth and centrally concentrated object, with no discernible spiral arm structure or distinct features such as prominent dust lanes. The morphology appears to be elliptical or lenticular, characterized by a generally spheroidal shape. There is a slight elongation, but the object is generally rounded in appearance. The color profile suggests a population of older stars, as the central region exhibits a yellowish hue, which is consistent with a passively evolving galaxy. There is no apparent evidence of ongoing or recent major merger events. The galaxy seems to be relatively undisturbed.
