The galaxy presents as a disk-shaped system, though some degree of disturbance is evident. The central bulge is prominent, displaying a yellowish hue, which may indicate an older stellar population. Extending outward from the bulge is a disk structure, appearing somewhat asymmetrical and loosely wound. There may be some level of warping present in the disk. Patches of bluer light are observed within the disk regions, indicative of younger, hotter stars. There seems to be some level of disruption occuring, based on the faint and diffuse emissions surrounding the main galaxy.
