The galaxy presents as a spiral, viewed at an oblique angle, with a clear disk structure exhibiting significant features. It appears relatively large on the frame, with an estimated diameter of approximately 10 arcseconds. The disk shows a noticeable warp. Dust lanes are prominent, especially on the side that is closest to edge-on. These dark features obscure the underlying starlight, indicating the presence of significant amounts of interstellar dust and gas. The galaxy exhibits evidence of minor disturbances likely due to gravitational interactions or past mergers. One side shows a bright, disturbed region with a hint of a tidal tail, while the other is relatively smooth. Color analysis shows it is bluer in its outer regions, indicative of ongoing star formation. There is no evidence of a dominant bulge.
