The galaxy presents a relatively smooth and featureless appearance. It exhibits an elliptical morphology, with a high degree of central concentration. The light distribution appears homogenous, lacking any distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, contributing to the galaxy's yellowish hue. There are no apparent signs of ongoing mergers or significant tidal disturbances. The overall structure indicates a galaxy that has undergone significant evolution and stabilization over time.
