The galaxy presents as a singular, concentrated structure. Its overall morphology appears largely spheroidal, lacking any readily discernible spiral arm structures or a pronounced disk component. The light distribution is relatively smooth and centrally concentrated. There is a slight asymmetry in the galaxy's shape, suggesting a possible interaction or minor disturbance event. The galaxy exhibits a yellowish hue, implying an older stellar population and reduced ongoing star formation. It has a substantial mass, and low amount of ongoing star formation.
