The galaxy presents as an elongated structure, likely a disk galaxy viewed at a high inclination. A prominent central bulge is visible, appearing relatively smooth and concentrated. The bulge exhibits a yellowish-red hue. The disk component displays a bluer color, indicative of younger stellar populations. The light distribution within the disk appears somewhat patchy, suggesting the presence of spiral arm structures or irregular star formation regions. The outer regions of the galaxy fade gradually into the background, indicating a smooth transition in stellar density. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major merger events or tidal interactions.
