The galaxy presents as an elliptical or lenticular system. Its overall form is smooth and featureless with an oblong shape, exhibiting a high degree of radial symmetry and a distinct lack of spiral arm structures. The galaxy's central bulge appears bright and concentrated, indicating a significant population of older stars. The surrounding disk is less luminous, possibly due to a lower density of stars or the presence of dust obscuring the light. There is a slight bluer tint in some regions, suggesting the presence of some younger stars in the system. Weak, elongated tidal features appear present, hinting at past interactions with other galaxies. Overall, the galaxy appears to be undergoing little recent star formation, suggesting a more evolved state.
