This galaxy appears to be a relatively face-on spiral galaxy, viewed at a slight angle. The central bulge is bright and somewhat amorphous, with a concentrated luminosity. Surrounding the bulge is a flattened disk structure. The disk appears smooth with little resolved structure, and the outer edges are less defined and more diffuse. There is a slight blue tint to the outer regions of the disk, suggesting the presence of younger, hotter stars in the spiral arms. Fainter reddish hues are noticeable near the core, which could indicate older stellar populations. The overall morphology suggests a spiral galaxy with a dominant bulge component and a relatively smooth, tightly wound disk.
