The galaxy presents as a lenticular, disk-shaped system viewed at a high inclination. A prominent central bulge dominates the morphology. The bulge exhibits a smooth, concentrated light profile, transitioning into a fainter, more diffuse disk. The disk shows a slight asymmetry. The overall color index suggests a mature stellar population, with the bulge appearing redder, potentially indicating older stars and less ongoing star formation compared to the disk. There's no visual evidence of strong spiral arms. The galaxy shows no obvious signs of active galactic nucleus activity or interaction with other galaxies.