The galaxy exhibits a clear spiral structure, with discernible arms emanating from a central bulge. The arms appear somewhat loosely wound, giving the galaxy a flocculent appearance. The bulge is moderately sized, with a concentrated bright core that suggests the presence of an active galactic nucleus or a dense population of stars. The galaxy is observed nearly face-on, allowing for detailed observation of its spiral structure.

The overall color of the galaxy indicates a mix of stellar populations. The central bulge exhibits a yellowish-orange hue, indicating the presence of older, redder stars. The spiral arms show a more bluish tint, implying ongoing star formation and the presence of younger, hotter stars. There is no apparent evidence of significant tidal interactions or major mergers in the galaxy's morphology. The disc appears relatively smooth and undisturbed, with no obvious signs of dust lanes or other major features. The galaxy appears to be a relatively isolated system, with no other galaxies nearby that could be affecting its structure or evolution.
