The galaxy presents as an edge-on spiral, with a notable central bulge. The disk appears thin and elongated. There is a clear distinction in color between the central bulge and the outer disk; the bulge displays a yellowish-white hue, suggestive of an older stellar population. The disk component shows a bluer tinge, possibly indicating younger stars and ongoing star formation. Dust lanes are faintly visible, particularly near the central bulge, obscuring some of the light. The galaxy lacks any prominent, well-defined spiral arms, which is consistent with an edge-on viewing angle. Overall, the galaxy's structure is fairly smooth, with no obvious signs of major recent mergers or interactions, although there may be minor disturbances within the disk.
