The galaxy presents as a centrally concentrated elliptical system, appearing largely featureless with a smooth light distribution. It has a generally round shape, but deviates slightly from perfect circularity. There are faint suggestions of disturbances in the outer regions, potentially indicating a minor interaction or merger event in its past. The core is a bright, yellow-orange hue, likely indicative of an older stellar population. A gradual decline in light intensity is observed outwards from the center, fading into the background sky. Star formation is likely low. 
