The galaxy presents as a relatively face-on spiral, exhibiting distinct spiral arm structure. Star formation is suggested by the blue color. The arms are moderately well-defined. A central bulge component appears small or virtually nonexistent. There is evidence of potential tidal distortions or merger activity affecting the galactic morphology. The galaxy's disk appears somewhat irregular, rather than a perfectly smooth rotation, indicating it may be involved in or recently have undergone an interaction. The galaxy appears in an active phase of stellar genesis. It looks to be barred spiral structure, but this may be from the tidal disruption.
