The galaxy presents as a spiral, with a notable central bulge of moderate size exhibiting a yellow-orange hue, suggesting an older stellar population. Faint spiral arms extend from the bulge, indicating the presence of ongoing star formation. The arms appear somewhat flocculent, with a relatively low concentration of intensely blue regions, pointing to a lower overall rate of star formation. Two main arms are visible, moderately wound around the bulge. There's a hint of asymmetry in the outer regions of the disk. There is no apparent interaction with any other large galaxies. The overall morphology indicates a disk galaxy at a moderate redshift.
