The galaxy appears to be a relatively smooth, elliptical type. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high stellar density. Moving outward from the core, the light diminishes gradually, with a smooth transition into the surrounding halo. There is a slight elongation to the galaxy's shape. No obvious spiral arm structures or dust lanes are readily apparent. The overall color appears to be slightly redder. There may be some minor disturbances, though it appears to be more or less undisturbed.
