The galaxy presents as a spiral type, viewed at a considerable inclination. The disk is visibly prominent, with a notable presence of spiral arms, though their definition is somewhat indistinct. The arms appear to exhibit a range of winding tightness, with a predominant presence of tightly wound structures, though some sections display a more open, medium-wound configuration. The central bulge is estimated to be relatively small to moderate in size. The galaxy exhibits a blue color, suggesting ongoing star formation. No presence of a strong bar structure is readily apparent. There is no visual indication of a major ongoing merger, however, there could be minor disturbances within the galaxy's structure.