The galaxy presents as an elliptical morphology, with a smooth and largely featureless appearance. The light distribution is centrally concentrated, exhibiting a radial falloff in intensity. The galaxy's color appears generally redder, indicating an older stellar population. The isophotes appear mostly round with little sign of disk structure or spiral arms, and no strong evidence of recent or ongoing merger activity is visible. Overall, the galaxy appears to be a relatively undisturbed, passively evolving system.
