The galaxy presents as an elliptical morphology. The light distribution appears smooth and centrally concentrated with a high degree of radial symmetry, lacking discernible spiral arms or a prominent disk. The galaxy's shape is elongated. A color gradient is observed, with the central region exhibiting a yellowish hue, suggesting an older stellar population, transitioning to a redder periphery. There is no indication of significant star formation, dust lanes, or tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
