The galaxy presents as a disk galaxy, viewed at an oblique angle. The disk structure is clearly discernible, with a brighter, more concentrated central bulge region. Spiral arms are visible. The arms appear loosely wound. There is evidence of a bar structure crossing the central bulge, and the bulge itself appears moderate in size. There is no obvious major or minor disturbance due to galactic merging. The overall color profile suggests a mixed stellar population, with some regions exhibiting bluer tints indicative of ongoing star formation.
