The galaxy presents as a centrally concentrated spheroid, exhibiting a high degree of smoothness. The light profile appears relatively uniform and lacks prominent spiral arm structures or a defined bar. The overall morphology suggests an elliptical galaxy, possibly of type E0-E3 due to the observed ellipticity. There appears to be a slight color gradient, with the central region appearing more red/yellow, potentially indicating an older stellar population. Fainter bluish regions are seen towards the galaxy outskirts, potentially indicating some low-level star formation. There is no obvious indication of ongoing major mergers or significant tidal disturbances. The galaxy's shape appears predominantly round.
