The galaxy presents a primarily smooth morphology. Its shape is generally rounded, with a slight elongation. A bright, concentrated central bulge is evident, exhibiting a yellowish-white hue. Surrounding this bulge is a fainter, more diffuse disk component. The disk displays a subtle bluish-green tint, potentially indicating the presence of younger stellar populations and ongoing star formation. There are hints of minor irregularities in the outer regions of the galaxy. There is no clear evidence of a major ongoing merger.
