The galaxy presents as a spiral, viewed at an angle that is not quite face-on, but more tilted. The arms are distinct and extend noticeably from the central bulge. The central bulge appears relatively small but with a moderate contribution to the overall light. The winding of the spiral arms appears to be moderately compact, with the majority of the arms being wound tightly, but some are moderately wound and loosely wound. There appears to be evidence of ongoing star formation as suggested by the bluer hues present within the spiral arms. A hint of an internal bar feature is visible crossing the central bulge. No major signs of a recent or ongoing major merger are visible, although the structure is slightly disturbed in at least one arm. The galaxy appears to be a relatively massive system.