The galaxy presents as a lenticular or early-type spiral, viewed at a high inclination. It appears relatively smooth in texture. A bright central bulge dominates the morphology, transitioning to a slightly flattened disk. Faint, diffuse spiral arm structures or dust lanes may be present, but resolution limitations make definitive identification challenging. The overall color is yellowish-white, suggesting an older stellar population with lower rates of star formation and reduced emission from ionized gas. There may be some minor asymmetry in the disk, potentially caused by a small perturbation. There is no visible evidence of an ongoing major merger event.