The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated with a gradual falloff in intensity towards its outer regions. The core exhibits a yellowish hue, potentially indicative of an older stellar population. There is no obvious spiral structure or distinct disk component visible. The galaxy's overall structure seems undisturbed, showing no signs of major mergers or tidal distortions. Faint, extended emission is barely perceptible surrounding the central region, suggesting a diffuse halo of stars.
