The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a smooth, centrally concentrated light profile. There is a bright, yellowish core region that dominates the visual appearance, indicative of an older stellar population. The overall shape is somewhat elongated, neither perfectly spherical nor a highly flattened disk, tending more towards an intermediate shape. Faint, diffuse extensions appear in the outer regions, suggesting a halo structure surrounding the brighter central components. There are no easily discernible spiral arm structures or significant dust lanes. The galaxy's colour gradient indicates redder colours toward the core, suggestive of more metal-rich, older stars concentrated in the center, with slightly bluer colours in the outer regions where younger stars may exist in lower abundance. There appear to be no signs of ongoing major merger activity or tidal disturbances; the structure is relatively undisturbed, with hints of only minor disturbances in the outer regions.
