This galaxy presents as a spiral galaxy with a relatively bright, compact central bulge. The spiral arms are well-defined, displaying a flocculent structure with what appears to be regions of active star formation. These star-forming regions are highlighted by their bluer color in the image, indicative of the presence of hot, young stars. There is evidence of winding in the spiral arms, with a moderate pitch angle observed. A small stellar population is visible, and some of the light has undergone redshift as it approaches the viewer. There are no signs of significant interaction with other galaxies or major disturbances.
