The galaxy appears to be a spiral galaxy, although the spiral arms are not very distinct. There is evidence of a bar structure bisecting the central bulge, it is quite prominent. The bulge dominates a good portion of the galactic structure, appearing moderate in size. The galaxy exhibits colors indicative of a mix of stellar populations, with the central bulge appearing more yellow or red, and the disk showing blue hues. This suggests ongoing star formation within the disk, while the bulge contains older stellar populations. There appears to be some disk warp. Overall, the galaxy seems to be relatively undisturbed with no major mergers visible. There is evidence of minor disturbances within the galactic disk.
