The galaxy presents a distinct morphology characterized by a prominent central bulge surrounded by a well-defined disk. The bulge exhibits a moderate size relative to the overall galactic structure and appears relatively smooth. Evident spiral arm structures emanate from the central region, showcasing a somewhat flocculent pattern. The disk component displays a moderate inclination, affording a partial view of the spiral architecture. There's no indication of any significant bar structure within the galaxy. Furthermore, visual assessment suggests no obvious signs of ongoing major merger activity. The galaxy's overall color profile indicates a mix of stellar populations, with a hint of ongoing star formation activity particularly in the spiral arms and disc region.
