The galaxy is a disk galaxy oriented nearly edge-on with respect to our line of sight. A distinct dust lane is visible, bisecting the galaxy along its major axis. The dust lane appears somewhat patchy and uneven in its distribution.

The central bulge is prominent and elongated, exhibiting an elliptical shape. The luminosity appears to increase steadily towards the center, with no distinct features like rings or bars visible. The bulge displays a slightly boxy morphology.

The disk is relatively thin and elongated. The outer regions of the disk appear fainter and more diffuse than the central bulge. There is no evidence of strong spiral arm structures or significant star-forming regions readily visible in the disk, likely due to the edge-on viewing angle.

No signs of a major ongoing merger are apparent. The overall morphology suggests a relatively undisturbed disk galaxy. Faint, subtle irregularities are potentially present in the outer disk, suggesting minor tidal interactions or internal disturbances.
