The galaxy presents as a spiral type, observed at a moderate redshift. Its structure exhibits two prominent spiral arms emanating from a central bulge region. The arms appear well-defined, demonstrating a winding pattern that transitions from medium to loose. The presence of a bar structure cannot be definitively ruled out due to image quality. The central bulge appears relatively small and not particularly dominant, suggesting it is either small or non-existent. The galaxy's light is largely concentrated in the arms and the central region, with a subtle blue hue indicating ongoing star formation. There are indications of possible interaction or minor disturbances. Overall, the galaxy is a spiral exhibiting ongoing star formation.
