The galaxy exhibits an overall elliptical morphology with a smooth light distribution. The central region is characterized by a concentration of yellow light. A fainter, blue-ish extension is observed emanating from the primary galaxy. It is difficult to discern any distinct internal structure or spiral arms. There may be some disturbance in the morphology, potentially indicating a minor interaction or merger event. The colour suggests the presence of both older stellar populations (yellow) and regions of ongoing, albeit relatively low, star formation (blue).
