The galaxy presents as a flattened, disk-shaped structure, viewed at an intermediate angle relative to its rotational plane. The central region exhibits a bright, concentrated luminosity suggestive of a prominent galactic bulge. Fainter spiral arm structures are visible extending outward from the central bulge, appearing tightly wound. These arms are somewhat flocculent, with less defined boundaries and a patchy distribution of star formation regions. Dust lanes are present, subtly obscuring portions of the disk and contributing to its mottled appearance. There are no obvious signs of a recent major merger event.
