The galaxy presents as a singular, relatively smooth, and concentrated object. It exhibits a near-spherical morphology. A notable absence of defined spiral arms or a prominent disk structure is observed. The galaxy's color profile suggests a stellar population that is not dominated by young, massive stars, but is composed of a mature population. There is no obvious presence of strong dust lanes or significant star forming regions, but a faint presence of star formation could still be present. The overall light distribution indicates that it is a galaxy with a high concentration of stars toward its center. There are no apparent signs of ongoing major merger events or significant tidal disturbances. 
