The galaxy presents a relatively smooth and concentrated morphology. It exhibits a largely featureless appearance with a high degree of central concentration. The galaxy's shape appears nearly circular, deviating minimally from a perfect sphere. The light profile demonstrates a gradual decline in intensity from the core to the outer regions. The galaxy appears to be a relatively quiescent system, potentially with a low star formation rate. There is no evidence of strong tidal interactions or ongoing mergers. The dominant light appears to be towards the redder end of the spectrum.
