The galaxy appears as a roughly elliptical structure with a centrally concentrated bulge. The color gradient suggests a higher concentration of older stellar populations in the core, which exhibits a yellowish-orange hue. Moving outward from the center, the disk reveals a bluer tint, indicating the presence of younger, hotter stars. The overall smoothness of the galaxy suggests that it is an early-type spiral or lenticular galaxy, although some faint, irregular structure is observed in the outer regions of the disk. There is no definitive evidence of spiral arms. There is a slight elongation of the galaxy shape, deviating slightly from a perfectly circular form. No major ongoing merger events are obviously visible; the galaxy appears relatively undisturbed with a quiescent morphology.
