The galaxy appears as a relatively smooth, elongated structure. Its morphology is consistent with a lenticular or early-type spiral galaxy, viewed at an oblique angle to our line of sight. The central bulge appears prominent and exhibits a bright, concentrated luminosity. Moving outward from the core, there is a gradual decrease in luminosity, with a somewhat diffuse halo extending beyond the main body. There is a hint of a disk component, but distinct spiral arms are not apparent, suggesting a more evolved or quiescent state. Overall, the galaxy presents a rather undisturbed morphology, with no obvious signs of a major merger or tidal interactions with neighboring galaxies.
