The galaxy presents as a relatively compact object with a smooth, featureless appearance. Its morphology suggests an elliptical or lenticular classification. There is little evidence of spiral arms, dust lanes, or active star formation regions within the observed wavelengths. The object appears moderately luminous. Color gradients are subtle, showing a slightly bluer core that transitions to a redder halo. The overall structure indicates a well-evolved system, likely dominated by an older stellar population.
