The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. It exhibits a yellowish-white core, suggesting a population of older stars. The outer regions transition to a bluer hue, hinting at the presence of younger stars and ongoing, albeit potentially low-level, star formation in the outer disk. The overall shape is somewhat elongated, though not drastically so; it is more lenticular than a highly flattened spiral. There is no obvious indication of significant spiral arm structure or major disturbances indicating recent merger activity. Faint, diffuse extensions are observed at the outer edges, but they are subtle and do not indicate a strong tidal interaction. The light appears to be smoothly distributed, reinforcing the impression of a settled, evolved system.
