This appears to be a spiral galaxy, viewed at an oblique angle. It exhibits a well-defined disk structure with prominent spiral arms. The arms are tightly wound in the central region of the galaxy. The central bulge is relatively small, though bright and somewhat elongated suggesting the presence of a bar feature within the galaxy's core. The spiral arms appear somewhat flocculent. There is evidence of ongoing star formation within the arms, indicated by the presence of some knots of bluish light. The galaxy shows some signs of disturbance, possibly minor interactions with other galaxies or internal instabilities. Overall, it presents a classic spiral morphology with signs of both ordered structure and localized star formation.
