The galaxy presents as a relatively smooth object with a concentrated central bulge. The overall shape is elliptical, tending toward a slightly flattened form. There is a noticeable radial color gradient, with the core appearing yellower and transitioning to a slightly bluer hue in the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. Minor disturbances are present, suggesting a possible past interaction, however it is most likely not merging. This system is massive and has a suppressed star formation rate, suggesting that the system is in the process of quenching. The surface brightness is highest at the center, indicating a high stellar density in the galactic nucleus.
