The galaxy presents as a spiral type, with discernible arm structures emerging from a central bulge. The spiral arms are somewhat flocculent, suggesting an irregular pattern. The disk appears relatively thin. The central bulge exhibits a moderate concentration of light. Evidence of a bar structure is ambiguous, but may be present. The overall color is consistent with a galaxy containing both older stellar populations and ongoing star formation, as indicated by the presence of both reddish and bluish hues within the arms. There are no obvious signs of major mergers, but there appears to be some kind of irregularity in the spiral structure which could suggest some kind of tidal interaction. The galaxy is viewed at a slight angle to face-on.
