The galaxy presents a generally smooth, featureless appearance, suggesting a relatively evolved system. The light profile appears concentrated towards the center, indicating a significant central bulge or nucleus. There is no apparent spiral structure or significant disk component visible. The color is somewhat uniform, with a subtle shift towards redder wavelengths in the central regions, possibly indicating an older stellar population. There is a minimal presence of blue light within the galaxy, suggesting low ongoing star formation. The overall shape appears generally round, lacking any strong indications of tidal disturbances or recent major mergers. Minor irregularities are present in the outer regions, which could point to ongoing or past minor interactions, though the system appears largely relaxed and undisturbed.
