The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core that appears yellowish-white in color, suggesting a population of older stars. Moving outward from the center, the light gradually fades into a diffuse halo. The galaxy is mostly homogenous in color, which indicates an older population of stars. The absence of prominent spiral arms or dust lanes, coupled with the smooth light distribution, further supports its classification as an elliptical galaxy. There might be slight perturbations or distortions in the outer regions, suggesting a possible interaction, but they are not particularly prominent. Overall, the galaxy appears to be a relatively undisturbed system, exhibiting properties consistent with a mature elliptical galaxy.
