The galaxy exhibits a disturbed morphology, suggestive of a recent or ongoing interaction or merger event. The overall structure presents a distorted disk-like appearance, but is ill-defined. While a spiral structure can be inferred, it is not prominent. The color distribution is non-uniform, with bluer regions indicating areas of active star formation. There appears to be a central concentration of light, possibly indicating a bulge component. There is evidence of tidal features or extended structures, particularly on the left of the galaxy, indicating significant gravitational interaction. Patches of dust may be present, though obscured by the star formation regions. A bar structure does not seem to be present within this galaxy.
