The galaxy presents as a relatively smooth, elliptical-like object with a high degree of central concentration. A bright, yellowish core dominates the structure, suggesting an older stellar population. There is a subtle radial color gradient, with the outer regions appearing slightly bluer than the core. No distinct spiral arms or significant dust lanes are apparent. Overall, the galaxy appears to be an early-type system with a largely homogenous stellar distribution and minimal ongoing star formation. There are no other visible signs of significant disturbance such as tidal tails or asymmetric morphology.
