The galaxy presents as a relatively smooth, centralized object with a concentrated luminosity profile. It appears elliptical in shape, with a high degree of roundness. There is a noticeable color gradient, shifting from a brighter, yellowish core to a more diffuse, reddish outer region. No distinct spiral arms or obvious dust lanes are visible. The overall structure suggests a well-mixed stellar population, potentially indicating an evolved system without significant ongoing star formation. There is no obvious evidence of any major merger events or significant tidal disturbances in the immediate vicinity. Minor disturbances cannot be ruled out. The galaxy's morphology indicates it is likely an elliptical galaxy, based on its smooth, featureless appearance.
