The galaxy presents as an elliptical-type object, exhibiting a high degree of central concentration. It appears largely featureless with a smooth light distribution. The isophotes appear to be somewhat elliptical in shape, tending towards a more oblate morphology rather than a perfect circle. Color gradients are subtle, transitioning from a yellow-white core to slightly redder hues in the outer regions, indicating potentially older stellar populations or the presence of dust in the periphery. No distinct spiral arms or prominent dust lanes are discernible, suggesting a lack of significant ongoing star formation. Overall, the galaxy appears to be a relatively quiescent system, likely a massive elliptical at intermediate redshift.
