The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. Its shape appears moderately rounded, showing deviation from a perfect circular form. The central region displays a concentrated, yellowish hue, indicating a possible population of older stars. Moving outwards, the galaxy transitions to a bluer color, suggesting the presence of younger stars. There are no immediately obvious signs of a major ongoing merger or significant tidal disturbance. The general smooth appearance and rounded shape indicates it is likely a relatively evolved system. 
