The galaxy presents as a flattened, disk-shaped system, seen at an almost edge-on orientation. Its color profile shifts from a yellowish core region to bluer hues towards the outer edges of the disk. The central bulge appears relatively small and concentrated. The disk structure appears smooth, with no obvious spiral arm features visible at this resolution and viewing angle. The outer edges of the disk appear less defined, with a gradual fading into the background sky. There appears to be a slight warp or asymmetry in the disk's outer regions. The overall light distribution suggests that the stellar population is slightly older in the bulge and gradually becomes younger with the outer edges.
