The galaxy presents a flattened, elliptical morphology. A central bulge region exhibits a pronounced orange hue, potentially indicative of an older stellar population and reduced star formation activity in that area. Moving outward from the core, there is a transition to a more greenish color in the disk region. The overall structure suggests that the galaxy has no prominent spiral arms or bar feature. The galaxy appears relatively undisturbed, lacking signs of ongoing major merger activity, although some minor distortions may be present. It's shape is more in between round and cigar shaped. 
