This galaxy exhibits a flattened, elongated morphology, strongly suggesting an edge-on or nearly edge-on disk orientation relative to our line of sight. The central bulge is relatively prominent, displaying a yellowish hue. There's a visible disk component that appears somewhat diffuse, with hints of bluer regions interspersed, potentially indicative of ongoing star formation. The overall structure seems relatively smooth, but with a slight disturbance or asymmetry in the distribution of light in the disk, possibly suggesting a minor interaction or internal dynamic process. The color gradient from the bulge to the outer regions of the disk suggests variations in stellar populations and dust content throughout the galaxy.
