The galaxy presents as a slightly elongated, lenticular or early-type spiral structure. It exhibits a prominent central bulge, appearing smooth and concentrated with a yellowish hue. The outer regions show a gradual decrease in brightness, with a faint, diffuse disk extending beyond the central bulge. There appears to be some subtle color variation, potentially indicating some low-level star formation within the disk, however the morphology is dominated by an older stellar population. There are no obvious signs of spiral arm structures or major disturbances, suggesting a relatively quiescent state. The galaxy's smooth overall appearance indicates it is relatively evolved.
