The galaxy presents as a spiral type, exhibiting a disk-like structure with a notable central bulge. Spiral arms are present, although their morphology suggests a tightly wound configuration. The arm count appears to be in the range of three to four distinct arms. A relatively small bulge is present within the galaxy's center. The galactic disk presents as slightly edge-on with a bright core in the center and a fainter glow in the disk. There is no evidence of a strong bar feature within the galaxy. Overall, the galaxy doesn't show evidence of major disturbances or significant ongoing merger activity.