The galaxy presents as a somewhat face-on spiral, exhibiting a bright, concentrated central bulge that appears yellowish in color. Surrounding the bulge, a less defined spiral arm structure is visible. These arms show a bluer hue, suggesting the presence of younger stellar populations and ongoing star formation. There seems to be a general smoothness to the overall structure, although subtle disturbances might be present. There does not appear to be a grand design spiral structure, rather it looks to be more flocculent. The galaxy appears to be relatively isolated, with no obvious signs of a major ongoing merger.
