The galaxy presents as a spiral type with a moderate bulge. Prominent spiral arms extend outwards, displaying a relatively tight winding pattern. The color distribution across the galaxy suggests ongoing star formation, particularly in the spiral arms, evidenced by bluer hues. The galaxy exhibits no obvious signs of major interactions or mergers, though minor disturbances are possible given the slight asymmetry in the arm structures. The central bulge appears smooth, surrounded by a disk component that contributes significantly to the galaxy's overall luminosity. The orientation is somewhat face-on, allowing for a good view of the spiral structure.
