The galaxy presents as a centrally concentrated, ellipsoidal structure. The core region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. The light becomes less concentrated outwards from the core.

The galaxy appears relatively smooth in texture with no obvious spiral arm structures or dust lanes visible within this image. The outer regions display a faint greenish halo, which could potentially be indicative of diffuse, ongoing, but minimal star formation or scattered light from the central region. There is no apparent signs of major mergers or significant tidal disturbances. The overall impression is that of a mature galaxy undergoing little active star formation.
