The galaxy presents as a relatively smooth, elliptical structure. Its color profile is predominantly yellowish-orange, with a brighter central region indicating a concentration of older stellar populations. There is no discernible spiral arm structure or dust lane obscuration visible. The galaxy appears to be relatively isolated, showing no strong signs of tidal interactions or ongoing mergers, though a very slight asymmetry in the outer isophotes suggests a possible past interaction. Its overall morphology indicates a quiescent system, likely characterized by a low star formation rate.
