This galaxy presents a generally smooth and elliptical morphology. The light distribution is concentrated towards the center, displaying a bright, unresolved core. The galaxy exhibits a gradient in color, with the central region appearing bluer compared to the outer regions which appear more red, indicating potentially older stellar populations at the outskirts. There is no obvious spiral arm structure or dust lane evident in the image. The galaxy's shape is more rounded than cigar shaped, but not completely circular. There are no indications of ongoing major merger events, although there is possibly a minor asymmetry or perturbation in the outer halo. This might suggest a possible past interaction. Overall, the galaxy appears to be a relatively quiescent system.
