The galaxy appears to be a spiral galaxy exhibiting a complex morphology. There is a noticeable disk structure, though it is not perfectly defined, with some indication of spiral arm features. The arms appear somewhat loosely wound. A bar feature is suspected through visual inspection, though indistinct. The bulge component appears to be relatively small compared to the disk. The overall luminosity of the galaxy suggests a sizable stellar population. There may be interactions or mergers occurring given the irregular morphology, suggesting some possible tidal features or disturbances. There is a presence of bluer star forming regions and redder, dustier regions.
