The galaxy presents an edge-on morphology, exhibiting a flattened disk structure. A prominent dust lane bisects the galaxy along its major axis, obscuring the galactic nucleus. The disk shows some texture and irregularities, suggesting potential substructure. There is a bright central bulge or nuclear region. Based on the color profile, there is a possible recent interaction event, but the image does not provide enough information to be absolutely certain. There might be a small possibility of tidal features or other merging evidence, but those features are faint and obscured by the dust. Overall, the galaxy appears to be a late-type spiral galaxy, with notable dust obscuration and potential signs of interactions.
