The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a somewhat elongated shape. Its light profile seems to lack prominent spiral arms or distinct features. The central region presents a bright, concentrated core, possibly indicative of an actively star-forming nucleus or an active galactic nucleus. Moving outward from the core, the light gradually diffuses, with a subtle gradient in color from slightly yellower hues in the center to slightly bluer hues in the outer regions, perhaps reflecting differing stellar populations. There is a small amount of disturbance to the shape, but generally appears to be a relatively relaxed structure, not exhibiting signs of a major ongoing merger. 
