The galaxy presents as a spiral, exhibiting a substantial disk. Spiral arms are readily visible within the disk. These arms appear well-defined and extend outwards from a central bulge region. The bulge is small relative to the overall size of the galaxy. There is a slight bar visible in the center of the galaxy. The galaxy is viewed at an angle, with an inclination towards the observer. The structure appears slightly disturbed, but is likely not merging with another galaxy. Dust lanes are observable within the spiral arms. The galaxy exhibits a bluer hue in its outer regions, and reddens toward the central regions.
