The galaxy presents as a flattened, disk-like structure seen nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, possibly indicating an older stellar population. The disk component appears elongated and significantly thinner than the bulge. It exhibits a bluer color than the bulge, possibly indicating younger stars. There is a slight asymmetry or minor warping present in one of the outer edges of the disk. No distinct spiral arm structures are clearly discernible in this image, possibly due to the edge-on viewing angle. The galaxy appears to be relatively isolated, showing no immediate signs of ongoing or recent major mergers, although there could be some minor disturbances.
