The galaxy presents as a single, coherent object with an overall elliptical morphology, albeit slightly elongated. Its core appears bright and concentrated, exhibiting a yellowish-white hue, possibly indicating a population of older stars. Fainter, bluish light surrounds the core, forming a diffuse halo. There is a hint of a disk-like structure, subtly offset from perfectly spherical. Minor disturbances may be present; subtle asymmetries or irregularities are visible in the outer regions. The galaxy appears to be relatively isolated.
