The galaxy appears to be an elliptical type, characterized by a smooth, featureless morphology. It exhibits a centrally concentrated light profile, appearing nearly round. The core region displays a yellowish hue, possibly indicating a population of older, redder stars. Moving outwards, the color gradually shifts to a slightly bluer tone, suggesting a component of younger stars in the outer regions, although the overall star formation rate appears to be low. No distinct spiral arms or bar structures are discernible. There are no obvious signs of tidal disturbances or ongoing mergers, suggesting that the galaxy is relatively isolated and undisturbed. The smooth, symmetrical appearance points towards an evolved system.