The galaxy presents as an edge-on spiral, characterized by a prominent central bulge and a flattened disk. The bulge exhibits a yellowish hue, indicating an older stellar population. The disk is primarily composed of fainter blue light, suggesting ongoing star formation.

The dust lane appears to be thin and indistinct. There is no evidence of recent merging events or significant tidal disturbances affecting the galaxy's morphology. The bulge appears round.
