The galaxy exhibits a prominent spiral structure, with two clearly defined arms extending outwards from the galactic center. These arms are loosely wound, displaying a somewhat diffuse appearance, indicating ongoing star formation within them. A significant central bulge is visible, suggesting a moderate to high concentration of older stars in the galaxy's core. There is a hint of a bar structure crossing the central region of the galaxy. The galaxy appears to be undergoing a minor gravitational interaction or disturbance, possibly with a companion galaxy, or a recent merger in its past, slightly disrupting its overall symmetry.
