The galaxy presents a prominent spiral structure, with well-defined arms emanating from a central bulge. The arms appear flocculent and exhibit a patchy distribution of star formation regions, indicated by bluish hues. The central bulge has an elongated, bar-like feature crossing its central region. The bulge exhibits a yellowish color suggesting an older stellar population, with a relatively small contribution to the overall galaxy brightness. The galaxy does not show any obvious signs of ongoing major mergers. There is slight warping, suggesting a minor gravitational interaction.
