The galaxy presents a roughly elliptical morphology with a smooth, diffuse appearance. A central bulge exhibits a concentrated yellowish-orange hue, suggesting an older stellar population. The outer regions show a gradual decline in surface brightness, with a faint blue tinge that becomes more apparent further from the core. No distinct spiral arm structures or dust lanes are discernible. The overall structure hints at a galaxy that may have undergone significant dynamical relaxation or a recent merging event, resulting in the observed spheroid shape and lack of prominent features. There is no visual evidence of a strong star formation activity within the galaxy. Minor disturbances can be found on the outskirts.