The galaxy presents as a spiral type, viewed at an oblique angle, exhibiting an elongated shape. A prominent dust lane appears to bisect the galaxy's central region, obscuring a significant portion of the stellar population. This suggests a relatively high inclination angle. The spiral arms are somewhat diffuse and exhibit a flocculent structure. The central bulge is relatively small and not very bright. There is evidence of possible tidal features or disturbances, possibly indicative of a past or ongoing minor merger event, that are present at the far end of the galaxy. The overall color suggests moderate star formation.
