The galaxy presents as an elliptical or lenticular type system. It appears largely featureless, lacking prominent spiral arm structures or distinct dust lanes. The light distribution suggests a centrally concentrated spheroid with a smooth gradient, indicating an older stellar population. Color indices show a bias towards redder wavelengths, which is consistent with a population of older stars. There might be a slight asymmetry in the outer halo, possibly indicative of minor tidal interactions or past merger events. Overall, the galaxy appears well-established and quiescent in its current state.
