The galaxy presents as an elongated, edge-on spiral with a prominent, centrally located bulge. The bulge exhibits a yellowish hue, possibly indicating a population of older stars. The disk is thin and extends outwards from the bulge, appearing flattened. The disk shows faint blueish tinges on the outer edges, hinting at some ongoing star formation. The overall dust lane signature is minimal, suggesting that it is either obscured by the edge-on orientation, or that it is not prominent. The galaxy's morphology is indicative of an undisturbed disk system that has not experienced any major recent mergers, as it shows no signs of significant tidal distortions or asymmetric features.