The galaxy presents as a spiral type, observed at an angle that is close to face-on. A prominent central bulge is apparent, contributing significantly to the overall luminosity. The spiral arms are well-defined, displaying a fairly ordered structure with a moderate winding, emanating outward from the central region. Two dominant spiral arms appear to be present. Patches of bluer light are present in the arms, and some faint red patches are visible as well. The bar is of an intermediate size but well defined. There are no obvious signs of ongoing or recent major merger events, although some minor tidal disturbance is possible.
