The galaxy presents as a disk galaxy, observed face-on. Prominent spiral arm structures are clearly visible, although somewhat tightly wound. These arms appear well-defined, extending outwards from a central bulge. The bulge component has a moderate size relative to the overall galactic structure. A bar-like structure also appears present across the central region. The galaxy exhibits a range of color variation, from a yellowish hue in the central bulge to more blueish tones in the spiral arms, potentially indicating ongoing star formation within the arms. The spiral arm count is difficult to distinctly identify, but it appears the galaxy may contain many spiral arms. There is no obvious indication of a recent major merger event, although minor disturbances cannot be ruled out. The disk appears not to be edge on.
