This galaxy appears to be a spiral galaxy, with a noticeable bulge and a disk structure that is tilted with respect to our line of sight. The bulge is relatively bright and appears yellow in color, suggesting an older stellar population. Faint spiral arms are visible, though they are not very well-defined and appear somewhat flocculent. The disk itself exhibits a bluer color than the bulge, indicating the presence of younger, hotter stars and ongoing star formation. There is no clear evidence of a recent major merger or strong tidal disturbances, although some minor asymmetries are seen. Based on these characteristics, the galaxy is likely undergoing relatively quiescent star formation within its disk, with the bulge dominated by older stars. Overall, the galaxy presents as a reasonably undisturbed spiral system at a moderate redshift.
