The galaxy presents a largely smooth and centrally concentrated morphology. It exhibits a roughly elliptical shape, appearing mostly round, with a slight tendency towards an intermediate spheroidal form. There is a smooth decline in brightness moving outward from the center. There is a dominant central bulge exhibiting a yellow-orange hue, potentially indicating an older stellar population with little active star formation. There is no clear evidence of spiral arms or a significant disk component. The galaxy's overall appearance suggests it is undisturbed, with no clear indications of recent or ongoing major merger activity. Subtly bluer tinges can be seen in the outskirts, suggesting very low levels of star formation may be ongoing. 
