The galaxy presents a generally smooth, rounded morphology. It exhibits a moderate degree of central concentration, with a diffuse halo extending outwards. There are some hints of asymmetry and what might be minor disturbances in its structure, suggesting a possible interaction or merger history, although a significant portion of classifications suggest no merger. Color gradients are observed within the galaxy; the central regions appear slightly redder than the outer regions. The overall color of the galaxy suggests a relatively evolved stellar population with ongoing, but low, star formation.
