The observed galaxy appears as a concentrated, elliptical structure with a smooth, relatively featureless morphology. The central region exhibits a bright, yellowish core, suggesting a high concentration of older stellar populations. The overall shape is slightly elongated, with a major axis that is longer than its minor axis. The galaxy's color profile transitions from the yellowish core to more reddish hues in the outer regions, potentially indicating a gradient in stellar population age or dust content. There is no clear evidence of spiral arms, dust lanes, or active star formation within this image. The smooth and rounded appearance supports classification as an elliptical galaxy.
