This galaxy appears to be a spiral galaxy at an intermediate redshift. The galaxy displays a prominent, moderately sized central bulge, which exhibits a yellowish hue, suggesting an older stellar population.

Extending from the bulge are spiral arms. These arms appear somewhat flocculent and are primarily blue in color, indicating the presence of ongoing star formation regions within them. These spiral arms are not tightly wound. 

There are no indications of a strong bar structure. The general morphology does not indicate any major ongoing merger events, though there may be a minor disturbance or irregularity.

The overall appearance is of a galaxy with a mix of both old and newly formed stars, with a substantial disk component.
