The galaxy presents as a spiral galaxy, oriented face-on relative to our line of sight. It exhibits a central, relatively bright bulge with a yellow-orange hue, suggesting an older stellar population. Fainter spiral arms extend outward from the bulge, displaying a bluer color indicative of ongoing star formation. These arms appear somewhat diffuse and moderately tightly wound. A faint disk is implied by the overall flattened structure, though it lacks a sharply defined edge. Evidence of a weak bar structure is subtle. There is no apparent sign of major disturbances or ongoing mergers, the galaxy's structure appears relatively well-defined and settled.
