The galaxy presents a generally smooth morphology with a concentration of light towards the center. The object appears ellipsoidal, with a high degree of roundness. There is evidence of possible tidal distortions, potentially indicating an ongoing or past interaction or merger with another galaxy. The galaxy exhibits a color gradient, with the central region appearing more yellow, suggesting an older stellar population and a lower rate of star formation compared to the fainter, slightly bluer outer regions. The overall structure is dominated by a bulge-like component, with no clear indication of spiral arms or a prominent disk. The galaxy displays a relatively compact size.