The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of radial symmetry. There's a bright, concentrated central bulge dominating the galaxy's luminosity. The galaxy lacks prominent spiral arm structures or significant dust lanes. It is generally round in shape. Faint hints of a disk structure may be present, but are not well-defined. There is no evidence of active galactic nuclei activity or substantial ongoing star formation. The galaxy appears to be relatively undisturbed, lacking signs of recent major merger events.
