This galaxy exhibits a prominent spiral structure. The arms are tightly wound around a bright, moderately sized central bulge. The color gradient suggests active star formation within the spiral arms, which display a mottled texture. This is indicative of both younger, bluer stars and dust lanes. The bulge appears relatively smooth and featureless. A weak bar structure may be present traversing the central region. The galaxy is oriented close to face-on with respect to our line of sight. There are no readily apparent signs of major mergers or significant tidal disturbances, though minor disturbances may be present.
