The galaxy appears as a centrally concentrated, spheroidal system, lacking any discernible spiral arm structure or prominent disk features. Its morphology is largely smooth, with a high degree of central concentration. The galaxy exhibits a noticeable color gradient, with a yellowish-white hue in the central region gradually transitioning to a bluer periphery. This suggests an older stellar population dominating the core, while younger, bluer stars may be more prevalent in the outer regions. The absence of any significant tidal features or distortions indicates that the galaxy is relatively undisturbed, showing no apparent signs of recent major mergers or interactions. The galaxy appears to be fairly isolated.
