The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth, spheroidal morphology. It displays a predominantly yellow-orange hue, indicative of an older stellar population. No distinct spiral arms or prominent dust lanes are discernible. There is a slight elongation in its overall shape, deviating from a perfectly circular form. The galaxy's light profile suggests a gradual fading from the bright central region towards the outer edges, lacking sharp boundaries. There are no apparent signs of major tidal disturbances or ongoing mergers. The galaxy is relatively compact in apparent size, and is likely a large elliptical galaxy. 
