The galaxy appears to be a spiral, however, it is difficult to distinguish defined spiral arms. It exhibits a relatively smooth, though somewhat irregular, structure. The central bulge is not sharply defined, blurring out toward the disk, and the galaxy's overall color suggests a mix of stellar populations, with some bluer regions indicative of ongoing star formation and redder regions potentially indicating older stellar populations. There is some slight asymmetry present, indicating there is a chance the galaxy is undergoing or has undergone an interaction of some kind. Overall, it seems that this object is relatively normal for a spiral galaxy.
