The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. The central region displays a concentrated yellowish hue, suggesting a higher density of older stellar populations. Moving outward from the core, a subtle transition to a bluish tint can be observed in the outer regions, possibly indicating pockets of younger stars or a recent minor merger event. The galaxy does not show any clear spiral arm structures, though there is a slight unevenness that indicates some mild disturbances or past interaction. The overall shape is somewhat elongated, leaning more towards an elliptical than a perfectly spherical form, suggesting that the object is an E3 or E4 galaxy.
