This galaxy presents as a spiral type with moderately defined spiral arm structures. The arms appear somewhat diffuse, lacking sharp definition, and exhibit a bluer color profile, which might suggest active star formation regions within them. The bulge component is not overly prominent, appearing relatively small compared to the disk. The disk itself has an intermediate inclination, revealing both spiral structure and a hint of a flattened shape. There might be a slight asymmetry or subtle disturbances within the galaxy's structure, hinting at possible past interaction or merging events. The overall color is bluish. The galaxy appears relatively isolated.
