The galaxy presents as a moderately inclined spiral or irregular system. There is some suggestion of a disk structure, but it appears perturbed. Evidence of ongoing or recent interaction is apparent, with morphological distortions visible. The central bulge is not prominent; light appears evenly distributed throughout the object, indicative of ongoing star formation across the galactic body. Color gradients are present, with bluer regions interspersed with yellower and redder areas. The lack of distinct spiral arm structure and the disturbed morphology suggest a complex dynamical history, possibly including mergers or tidal interactions.
