The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. The light is concentrated toward the center, indicating an older stellar population. There is a hint of a disk-like component, but it is not well-defined. A faint, extended halo surrounds the main body of the galaxy, which might be indicative of tidal interactions, or star formation. There are few visible signs of significant star formation, such as bright blue regions or prominent dust lanes. The overall morphology suggests an early-type galaxy with little ongoing star formation.
