This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a generally round morphology, with a slight deviation from perfect circularity. The galaxy presents a yellowish-orange hue, suggesting an older stellar population and potentially a lower rate of current star formation. There is no apparent spiral structure or distinct disk component visible. It is characterized by a concentrated central region with a gradual decrease in luminosity towards the outer edges. There are indications of a possible minor disturbance in the morphology. The overall structure is relatively uniform, consistent with an evolved galaxy.
