This galaxy presents as a luminous, relatively compact object with a noticeable elliptical morphology. The core region exhibits a concentrated, bright yellowish hue, suggesting an older stellar population. A fainter, bluish extension is observed on one side, possibly indicating a region of more recent star formation or perhaps an ongoing interaction with another galaxy. Overall, the galaxy appears to be a transitioning system, possibly moving towards a more quiescent state following a period of significant activity. Further spectral analysis is recommended to confirm star formation rates and age gradients within the observed structures.
