The galaxy presents a somewhat elliptical morphology, appearing mostly smooth with some suggestion of extended features on one side. The central bulge is prominent, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. A subtle color gradient appears, shifting towards a bluer tone away from the core which might suggest more recent star formation in the outer regions. The overall light distribution implies that the object is fairly well concentrated with a fraction of ongoing or recent merger activity. The object has a mass of approximately 10^10.8 solar masses and moderate levels of star formation. 
