The galaxy presents as a centrally concentrated elliptical morphology. It exhibits a smooth, diffuse light profile with no obvious spiral arm structures or dust lanes visible. The core appears bright and slightly yellowish, suggesting an older stellar population dominates the central regions. There is a gradual decrease in light intensity moving outward from the core, transitioning to a more reddish hue in the outer regions, which may indicate a mix of older and cooler stars at the periphery. The overall symmetry of the galaxy suggests it is relatively undisturbed, lacking any signs of major mergers or tidal disruptions. The roundness and smooth features are prominent, indicating a high probability of it being an elliptical galaxy viewed from a perspective that does not show significant disk features.
