The galaxy presents as a spiral type, viewed at an angle that is nearly face-on. A distinct disk structure is observed, exhibiting a complex arrangement of spiral arms. These arms appear fairly well-defined. The central bulge is moderately sized and exhibits a somewhat concentrated luminosity profile. Color gradients are present, with the central bulge appearing more yellowish, and the spiral arms exhibiting bluer hues suggesting ongoing star formation. There appears to be some asymmetry present in the distribution of light within the disk, perhaps due to minor gravitational interaction with another galaxy. Evidence of a bar structure is weak or not apparent from the image.
