The galaxy exhibits a morphology consistent with a late-type spiral, presenting a discernible disk structure. Faint spiral arms are visible, appearing tightly wound around a prominent central bulge. The bulge appears moderately sized relative to the overall disk. Color gradients suggest active star formation concentrated within the spiral arms, showing bluer hues. Dust lanes are not clearly visible, but may be present and obscuring the light within the spiral arms. The galaxy displays a fairly face-on orientation. There are no obvious signs of major mergers, although minor disturbances cannot be ruled out at this resolution. The general shape is elliptical and fairly compact.
