The galaxy presents a largely smooth morphology, with a high degree of central concentration. The overall shape is roughly elliptical, displaying a high degree of roundness with no apparent bar structure. The color profile indicates a possible red-sequence galaxy with hints of bluer star formation regions. There is no obvious evidence of spiral arms or other disk-like features. No tidal tails or other major disturbances are observed, suggesting that the galaxy has likely not undergone a recent major merger. The galaxy appears to be in a relatively quiescent state, with a moderately high stellar mass.
