The galaxy presents as a flattened, disk-like structure viewed at a high inclination angle, approaching edge-on. Its central region exhibits a brighter, more concentrated luminosity profile, suggestive of a bulge component. The disk appears relatively smooth and uniform in color, displaying a yellowish-white hue. There is a hint of dust lane obscuration along the apparent major axis, particularly near the extremities of the visible disk, which contributes to a slight reddening of the light in those regions. Overall, the galaxy appears to be a quiescent system, with no obvious signs of recent major mergers or significant star formation activity.
