The galaxy presents as a spiral type. It displays a noticeable disk structure. The spiral arms are well-defined, exhibiting a tightly wound morphology. A central bulge is discernible; it appears to be of moderate size relative to the overall galactic structure. Evidence suggests ongoing star formation, observable from the bluer regions within the spiral arms. The galaxy exhibits a slight inclination. There does not appear to be any presence of a strong bar or major merger events.
