The galaxy presents a clear spiral structure, viewed at an oblique angle to our line of sight. Multiple spiral arms extend outwards from a central bulge region. The arms appear tightly wound, exhibiting numerous bright knots of star formation, tracing out a complex pattern. The bulge region exhibits a moderate brightness, and the arms are noticeably bluer in color compared to the central region. The bulge appears slightly elongated, possibly indicating the presence of a weak bar structure within. The galaxy does not show any major signs of a major merger or strong tidal disturbances, though minor irregularities in the arm structure could suggest minor gravitational interactions.
