The galaxy presents a flattened, elongated disk structure, indicative of a spiral or lenticular morphology seen edge-on or at a high inclination. A bright, concentrated central bulge is visible, displaying a yellowish hue suggestive of an older stellar population. Moving outward from the bulge, the disk exhibits a bluer color, hinting at ongoing star formation within. The overall color gradient suggests a spatial separation of stellar populations. The galaxy appears relatively undisturbed, showing no obvious signs of a major merger event, although a minor asymmetry could be present, indicating a possible interaction or past disturbance.
