The galaxy appears as a somewhat elliptical, centrally concentrated object. Its color profile indicates a potentially older stellar population, with light across g, r, and z bands that, while relatively faint, is more prominent toward the redder end of the spectrum. There is a hint of a disturbance on its lower end, perhaps from a minor tidal interaction or a faint jet. There is a bright, roughly central bulge with a surrounding halo that fades away with distance from the center. The outer regions are amorphous and lack a defined spiral structure.
