The galaxy presents as a spiral galaxy, observed nearly edge-on. The disk is the dominant feature, displaying a flattened profile. Traces of spiral arms are visible, appearing relatively diffuse and loosely wound. The presence of two dominant arms is suggested. A central bulge is present, appearing moderately sized. The bulge exhibits a yellowish hue, suggesting an older stellar population. No clear evidence of a strong bar is apparent. There are no indications of major merger activity but some minor disturbances may be present.
