The galaxy presents as a disk-dominated system, viewed nearly edge-on. There is a prominent central bulge that appears somewhat rounded. The disk shows limited resolution of distinct spiral arms or significant star-forming regions. The integrated light suggests moderate ongoing star formation. The galaxy's morphology appears relatively undisturbed, with no clear signs of major mergers or tidal interactions. It exhibits a high degree of symmetry and coherency. There is a slight boxiness observed in the bulge.