The galaxy presents as a luminous, elliptical-shaped object, exhibiting a smooth, concentrated morphology. The central region displays a high degree of brightness, with light gradually diminishing towards the outer edges. There is a general lack of distinct structural features such as spiral arms or a prominent disk. The color profile indicates a possible composition of older stellar populations, potentially with ongoing, but not extensive, star formation. Faint irregularities are present around the galaxy, suggesting a possible minor interaction or disturbance. The galaxy appears relatively isolated, showing no signs of a major merger event. Overall, the galaxy is consistent with an evolved system, possibly transitioning towards a quiescent state.
