The galaxy presents as a somewhat face-on spiral, although its structure appears relatively smooth and diffuse. There is a bright central bulge that appears almost spherical, suggesting a concentration of older stellar populations. The spiral arms are not well-defined; rather, there are broad, hazy areas that may indicate regions of star formation activity or perhaps a more flocculent spiral arm structure. The overall color is slightly blue, potentially indicative of recent or ongoing star formation. However, the color gradients are subtle and the galaxy does not appear to be actively forming a lot of stars. No obvious signs of a major merger event such as tidal tails or strong distortions are apparent, although there is a slight asymmetry in the overall shape, possibly indicating minor interactions or internal instabilities. The galaxy appears to be of moderate size.
