The galaxy presents a morphology consistent with a spiral type. Prominent spiral arms are observed, exhibiting a largely two-armed structure. The winding of these arms appears to range from moderately wound to loosely wound. A central bulge is apparent, estimated to be moderate in size relative to the overall galactic disk. A weak bar structure may be present in the central region. There is no indication of a recent major merger event or significant tidal disturbance, though there is some evidence of minor asymmetry, possibly suggesting minor interactions. Overall, this galaxy exhibits characteristics indicative of ongoing star formation and a disk-dominated morphology.
