The galaxy presents as a relatively compact, elliptical system with a smooth appearance. It exhibits a predominantly yellow-orange hue, suggesting an older stellar population with fewer ongoing star formation events. The light distribution is centrally concentrated, becoming fainter towards the outer edges. There is no evidence of prominent spiral arms or a well-defined disk structure. However, it appears to show some merging or interaction with smaller objects. The galaxy's morphology indicates it is in the process of merging.
