The galaxy presents as a spiral type, with tightly wound spiral arms emerging from a moderately sized central bulge. Two primary arms are discernible, though other arm fragments may be present. The arm structure is somewhat flocculent in appearance. There is a slight asymmetry in the overall shape of the galaxy. The central bulge exhibits a yellowish hue, which is potentially indicative of an older stellar population. The spiral arms appear bluer, suggesting ongoing star formation. There is no obvious evidence of a strong bar structure, but there could be a weak bar present. No obvious signs of interaction or major merging events are visible, although subtle tidal features or minor disturbances cannot be ruled out with the current image resolution.
