The galaxy presents as a flattened, disk-shaped structure, viewed nearly edge-on. It exhibits a noticeable bulge concentrated toward the center, with a smooth, rounded morphology. The disk is elongated, with a high degree of flattening. The color gradient suggests a yellow-red hue emanating from the central bulge, which transitions to a bluer tint at the outer edges of the disk. The overall light distribution appears smooth, indicating a well-established stellar population with potentially low levels of ongoing star formation observed within the disk, if any. The galaxy's structure appears undisturbed, showing no evidence of major mergers or tidal disruptions.
