The galaxy presents as a relatively smooth, elliptical-like structure, with a high degree of central concentration. The color profile indicates a dominance of older stellar populations, exhibiting a yellowish hue throughout the main body. There is no strong evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a relatively quiescent galaxy with a low ongoing star formation rate. The isophotes appear largely regular, showing no clear signs of recent major mergers or tidal disturbances, although there is the possibility of a minor disturbance to the structure of the galaxy. 
