The galaxy presents as a spiral galaxy exhibiting a prominent disk structure viewed at a slight angle. The disk shows evidence of spiral arm morphology, although the arms are not sharply defined. The central bulge appears relatively small compared to the overall disk size, and exhibits a brighter, more concentrated luminosity, hinting at a higher stellar density. The galaxy appears relatively smooth in appearance with a slightly elongated shape, showing an ellipticity of approximately 0.7. Color gradients suggest active star formation within the spiral arms, with bluer hues indicating younger stellar populations. Fainter, diffuse light extends beyond the main body of the galaxy, forming a halo. There are some irregular disturbances in the outer disk, suggesting potential interactions or ongoing merger events.
