The galaxy appears as a relatively smooth, elliptical object. The light distribution suggests a centrally concentrated structure with a gradual decrease in intensity outward from the core. The object is nearly circular in appearance, with a high degree of symmetry. The galaxy exhibits a yellowish-white hue in its central regions, possibly indicative of an older stellar population. A small area of red shift could also be seen on the periphery of the galaxy. The galaxy's overall morphology suggests it is likely an early-type galaxy, potentially an elliptical, with minimal signs of ongoing star formation, but some may exist. There is no obvious evidence of significant dust lanes or spiral arm structures within the image. A possible interacting galaxy or foreground object exists in the vicinity, given its distinct color.