The observed galaxy presents a distinct disk-like morphology, viewed at a moderate inclination. Prominent spiral arm structures are evident, exhibiting a classical two-armed pattern. The arms appear moderately wound. A bar structure traverses the central region of the galaxy, appearing strong and well-defined. A small bulge component is observed. Star formation appears ongoing within the spiral arms, evidenced by the presence of localized regions exhibiting bluer colors. The overall color index suggests a dominant population of relatively young stars. There is also a smaller galaxy nearby. The relative position and morphology might indicate a possible gravitational interaction or merger event in the distant future.
