The galaxy presents as a relatively smooth, elliptical-like structure. There is an apparent central bulge, which exhibits a strong concentration of light. The color gradient suggests that this central region hosts an older stellar population. The outer regions of the galaxy are less defined, with a gradual decrease in luminosity. There does not appear to be any strong evidence of spiral arms, distinct dust lanes, or ongoing major merger activity in this image, though there is slight disturbance in the morphology. The galaxy appears largely undisturbed and relatively relaxed in its morphology.
