The galaxy presents as a somewhat elliptical, face-on or nearly face-on system. The core region exhibits a notably concentrated luminosity, appearing bright and slightly reddish in color. A more diffuse, bluer halo surrounds this central bulge, suggesting the presence of a stellar population with a range of ages. There's a subtle indication of a disk structure, but it's not sharply defined. Faint disturbances can be observed that may hint at a recent minor interaction or merger event. The overall morphology suggests a galaxy that is transitioning between a late-type spiral and an early-type elliptical, but is mainly smooth.
