The galaxy presents as a relatively faint, disk-shaped structure, viewed edge-on. The central bulge is a bright, concentrated region, exhibiting a yellowish hue. The disk is more extended, displaying a bluer coloration towards the outer edges, suggesting the presence of younger stellar populations or active star formation within the spiral arms. There are some signs of dust lanes along the central plane of the disk, visible as subtle dark features against the brighter background light. The overall structure appears relatively undisturbed, with no obvious signs of recent major merger events or tidal interactions. The galaxy exhibits a relatively high degree of flattening, indicating a significant rotational component.
