The galaxy exhibits a generally smooth morphology with a central bulge that appears moderately concentrated. Its shape is roughly elliptical, displaying a slight elongation. There is a faint indication of a disk-like structure within the galaxy. Some minor disturbances in its morphology are possible. It has an absolute magnitude in the optical bands indicating that it is a luminous galaxy. The stellar mass is estimated to be high, suggesting that it is a relatively massive galaxy. The star formation rate is low, indicating that it is likely a galaxy transitioning from a more active star-forming phase to a more quiescent phase.
