The galaxy presents as a lenticular system with a relatively smooth morphology. It displays a pronounced central bulge, exhibiting a bright, concentrated luminosity. Faint, disk-like features appear to surround the bulge, though these structures are poorly defined. A slight asymmetry can be observed in the outer regions, possibly indicating minor gravitational interaction. Color gradients suggest a population of older stars dominating the bulge, whereas the disk shows hints of more recent star formation. No strong spiral arm structures are discernible. The overall form is generally uniform, though low level disturbances may be present. The galaxy presents a compact structure, spanning roughly 3 kiloparsecs.
