The object appears to be a spiral galaxy with a relatively bright, compact central bulge. The spiral arms are well-defined and exhibit a tightly wound morphology. There is some indication of a bar structure extending through the center of the galaxy. Based on the symmetry and well-defined arms, there are no obvious signs of major mergers or significant tidal disturbances. The presence of spiral arms suggests ongoing star formation within the disk. The bluish color in the spiral arms is consistent with the presence of hot, young stars. The prominence of the central bulge indicates that it is likely to be of moderate size, compared to the overall dimensions of the disk.
