This galaxy presents as a spiral with relatively distinct, well-defined arms. There is some clumping and granularity along the spiral arms, indicating regions of active star formation. The central bulge of the galaxy appears moderately sized and is bright, yellow and relatively smooth. The spiral arms are fairly tightly wound around the core. There does not appear to be a significant bar structure present. There's no visual evidence suggesting a major ongoing merger event or significant tidal disturbances. The galaxy disk itself presents nearly face-on to our view.