The galaxy appears as a flattened, elongated structure, indicative of a disk-like system viewed at a high inclination. The central region exhibits a bright, concentrated bulge, possibly suggestive of an older stellar population dominating the core. Proceeding outward, the galaxy displays a fainter, more diffuse disk. The disk exhibits a slightly blueish hue in the outer regions. The lack of pronounced spiral arm structures suggests a relatively smooth stellar distribution. There is no obvious sign of a major merger, but some small disturbances can not be fully ruled out based on the image.
