The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. The central region exhibits a concentrated luminosity with a color index suggesting an older stellar population. The color becomes slightly bluer at the edges. There is a faint halo surrounding the core. There are no apparent spiral arms or significant dust lanes. The overall structure indicates a relatively evolved system, likely with a considerable stellar mass and a low star formation rate. There is a slight hint of possible tidal disruption, suggesting this galaxy may have gone through a merger event.