The galaxy appears as an edge-on spiral, characterized by a distinct, elongated shape. There is a central bulge, which appears to be smoothly rounded. The disk shows some internal structure, though it's difficult to distinguish spiral arms clearly given the edge-on perspective. The galaxy exhibits a color gradient, with the central bulge having a yellowish hue, possibly indicating an older stellar population. Progressing outward along the disk, the colors appears to gradually shift towards redder tones, suggesting the possibility of dust lanes or varying stellar populations. The overall morphology seems undisturbed, with no obvious signs of recent major mergers or tidal interactions.
