The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated core, suggesting a substantial central mass concentration, potentially a supermassive black hole. Moving outwards from the core, the light gradually diminishes, transitioning to a diffuse halo. The galaxy appears relatively undisturbed, with minimal evidence of tidal interactions or major mergers. There is a slight elongation in its shape, with the galaxy being neither perfectly circular, nor a cigar-shaped galaxy. Faint blue hues in the outer regions hint at ongoing star formation. The galaxy appears to be a moderately sized object with a fairly moderate star formation rate.
