The galaxy presents a largely smooth, elliptical morphology with a dominant central bulge. It exhibits a high degree of rotational symmetry, appearing nearly circular. There is a slight elongation, but no distinct spiral arm structures or bar features are discernible. The galaxy's light profile appears centrally concentrated, fading gradually towards its edges. Color gradients are subtle, with a slightly bluer hue in the central region that fades to a redder color towards the outer halo. There is no clear evidence of ongoing major merging activity, although some minor disturbance may be present within the halo. Overall, it appears to be a relatively evolved galaxy.
