The galaxy presents a smooth, elliptical morphology. It appears predominantly featureless, lacking discernible spiral arms or a prominent disk structure. The light distribution suggests a high degree of central concentration, with brightness decreasing steadily outward from the core. There's a subtle color gradient visible, transitioning from a yellowish core to a slightly redder halo, potentially indicating a change in stellar population with radius. The galaxy appears largely undisturbed, with no obvious signs of recent merger activity or tidal interactions. Based on the apparent roundness and the light profile, the galaxy is consistent with an elliptical classification, potentially an E0-E3 type.
