The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Evident spiral arm structure is observed, displaying a relatively tightly wound morphology. A central bulge is apparent, occupying a relatively small proportion of the overall galactic structure. There is no strong bar structure, however a faint one may be present. The spiral arms appear to exhibit a flocculent texture. No signs of major disturbances or ongoing mergers are immediately evident, although a minor asymmetry in the outer disk might suggest past or ongoing interactions. Based on its color, it is likely undergoing moderate star formation activity.
