The galaxy appears as a centrally concentrated, disk-like structure. The core region exhibits a bright, yellowish-white glow, suggesting a high density of older stellar populations. This bright central bulge appears to be fairly smooth, with a generally elliptical shape that transitions smoothly into a fainter, flattened disk.

The disk is oriented edge-on relative to our line of sight, which obscures any potential spiral arm structure. The edges of the disk exhibit some subtle color variation, but the overall appearance is fairly homogenous. The galaxy shows no obvious signs of significant interaction or major disturbances in its morphology. There is a faint, red band through the center of the galaxy, indicating the likely presence of a dust lane that obscures light.

