The galaxy presents a somewhat irregular, yet discernible spiral structure. The spiral arms appear moderately wound, suggesting an intermediate type between a tightly wound spiral and a flocculent spiral galaxy. These arms exhibit a slightly clumpy morphology, hinting at the presence of ongoing star formation regions within the disk. The central bulge is prominent, exhibiting a strong concentration of light, indicating a significant stellar population, likely composed of older stars. The galaxy displays a blueish tint, with an increasing concentration of white in the center. There is a possible faint bar structure that runs through the bulge. There are noticeable disturbances, indicating signs of a potential minor galactic interaction or ongoing merging event in the galaxy's recent history. The galaxy appears moderately inclined with an elongated shape.
