This galaxy presents as a spiral type, viewed at a slight angle to face-on. Spiral arm structures are clearly visible, showing a relatively high degree of organization. The arms appear somewhat flocculent rather than tightly wound, and exhibit varying degrees of blueness which indicate regions of active star formation. There is a significant central bulge component; the size of the bulge is moderate in comparison to the overall disk. A central concentration of light is apparent, with a yellowish color. The galaxy appears to be relatively isolated with no signs of major mergers or interactions. The color indices indicate ongoing star formation but not at extremely high rates.
