The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, diffuse light distribution. The core is bright and yellowish-white, indicating a significant population of older stars. There's a gradual decline in luminosity from the core outwards to the more diffuse, fainter outskirts. The overall shape tends towards a slightly elongated form but otherwise seems largely spheroidal. There is evidence of a disk component. Color gradients suggest a complex stellar population, possibly with ongoing, albeit low-level, star formation activity. There are no obvious signs of tidal disturbances or major mergers, suggesting a relatively isolated evolutionary history or a well-mixed merger remnant.
