The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the light becomes fainter with a subtle shift towards bluer colors, possibly indicating the presence of younger stars in the outer regions. There is no strong evidence of spiral arms or a distinct disk structure. The shape is largely circular, though there's a slight elongation discernable. The overall light distribution appears relatively undisturbed; there are no prominent tidal tails or signs of a major merger event. However, subtle irregularities in the outer regions may hint at a past interaction, perhaps a minor disturbance.
