The object appears to be a spiral galaxy, observed at a redshift of approximately 0.177. It exhibits a prominent central bulge surrounded by a disk structure. The bulge displays a yellowish hue, indicative of an older stellar population, while the disk shows bluer colors suggestive of ongoing star formation. Two main spiral arms are discernible, winding moderately tightly around the central bulge. Evidence of a bar structure is present, though it is not strongly defined. The disk does not appear to be edge-on, indicating a relatively face-on orientation with respect to our line of sight. There's no clear indication of a major ongoing merger, however some subtle disturbances may be present in the outer regions of the disk.