The galaxy appears to be a spiral type, although somewhat irregular. There are indications of disrupted morphology, particularly in the distribution of its light. A prominent disk is observable, displaying evidence of spiral arm structures, though these are ill-defined and appear flocculent. The central bulge is not a clear feature; it does not dominate the structure, perhaps it is small, or even absent. The galaxy exhibits an elongated shape. There may be the beginning stages of a tidal tail. There is evidence of some merging or interaction with another galaxy. The bluer color suggests active star formation regions throughout.
