The galaxy presents as a spiral, though not perfectly face-on. The central bulge appears significant, with a moderate size relative to the overall disk. Evidence of spiral arms is noticeable, albeit somewhat diffuse. The overall color gradient suggests a population of older stars dominating the bulge, transitioning to bluer hues in the outer disk, possibly indicating regions of on-going or recent star formation activity within the spiral arms. A slight asymmetry is observed in the disk. There is a hint of a bar-like structure bisecting the central bulge, though it is not sharply defined.
