The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular classification, exhibiting a centrally bright core that fades gradually into a more diffuse halo. There is a hint of a disk-like structure, but it appears relatively featureless. The galaxy's shape deviates slightly from perfectly round, leaning more towards an in-between or possibly slightly elongated form. Indications of a minor disturbance are present. The overall color is suggestive of an older stellar population, with a yellow or red-shifted appearance.
