The galaxy appears as an elliptical or lenticular system, exhibiting a largely smooth morphology with minimal signs of spiral arms or significant disk features. It is characterized by a moderate degree of roundness, though a slight elongation is also apparent. There are no immediately obvious signs of major mergers or significant tidal disturbances. The overall color profile suggests a relatively mature stellar population. Based on its luminosity, a substantial stellar mass is implied, and it seems there is ongoing moderate star formation.
