The galaxy presents a largely smooth, elliptical morphology. It appears well-defined, with a concentrated central region and a gradually decreasing luminosity gradient toward the outer edges. The core exhibits a bright, yellowish hue, suggesting an older stellar population and minimal active star formation. The surrounding halo is more diffuse, displaying a subtle transition to a greenish color, possibly indicating a sparse distribution of younger stars or ionized gas. No distinct spiral arms, bars, or significant dust lanes are discernible, supporting a classification as an elliptical galaxy. The overall appearance is consistent with a massive, evolved system, showing little evidence of recent major mergers or significant disturbances. A small percentage of artifacts are present in the image and there is a small chance that there is some merging happening in the galaxy. The round shape of the galaxy also leads to the theory that it is an elliptical galaxy.
