The galaxy presents as a smooth, elliptical-shaped object with a concentrated central bulge. The light distribution suggests an older stellar population, indicated by the yellowish-orange hue of the core. The outer regions exhibit a gradual decline in luminosity, lacking distinct spiral arm structures or prominent dust lanes. The overall morphology implies a relatively evolved system, potentially undergoing little active star formation. Slight asymmetry in the outer isophotes hints at a possible past interaction, but no major merging event is currently apparent. The galaxy's form is more elongated than perfectly circular.