The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its overall color is yellowish-orange, suggesting an older stellar population with fewer young, blue stars. The central bulge is well-defined and appears bright and concentrated. There is a faint disk component with hints of spiral structure that appear as slight disturbances within the disk. There are no obvious signs of a major ongoing merger, although subtle asymmetries could indicate a minor interaction or past merger event. 
