The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. It presents a predominantly yellow-orange hue, suggesting a stellar population dominated by older, cooler stars. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The galaxy's overall shape is generally round, with only slight deviations from perfect circularity. No significant signs of ongoing merging events or major tidal disturbances are visible. There appears to be limited star formation.