The galaxy presents an elliptical morphology, with a smooth, featureless appearance. It exhibits a concentrated central bulge that radiates intensely. The luminosity gradually decreases outwards from the core, lacking any distinct spiral arm structures or prominent dust lanes. Its overall color is predominantly yellowish-orange, indicative of an older stellar population. There are no signs of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, with a single nearby companion galaxy of lower luminosity. The overall impression is that of a mature, quiescent system with a minimal rate of star formation.
