The galaxy presents a distinct spiral morphology, exhibiting two prominent and well-defined spiral arms. These arms appear relatively loosely wound, extending outwards from a central region that displays a moderate bulge component. The bulge does not dominate the galaxy's overall structure. The central region appears somewhat elongated, suggesting the presence of a weak bar structure, possibly oriented horizontally in this image. There is little evidence of flocculent structure, or tightly wound arms. The color of the galaxy appears somewhat blue.

There's no evidence of a major ongoing merger; however, subtle irregularities in the spiral arm structure hints a potential minor interaction or disturbance. Overall, this is a spiral galaxy with a noticeable disk component, a modest bulge, and loosely wound spiral arms, exhibiting a sign of a weak bar.
