The galaxy appears to be a relatively smooth and rounded system. Its color is predominately yellow-orange, indicating an older stellar population with fewer hot, young, blue stars. There is a bright, concentrated central bulge. No distinct spiral arms or prominent disk features are visible, suggesting it may be an elliptical galaxy or a lenticular galaxy seen face-on. There is no indication of a major ongoing merger event, although there might be some minor disturbances in the outer regions. Based on the apparent size and redshift, this is a reasonably large galaxy at a considerable distance. Its estimated mass appears significant.
