The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a distinct disk. The light distribution appears concentrated towards the center, suggesting a high degree of central mass concentration. There is a subtle color gradient, with a slightly bluer hue towards the outer regions, potentially indicative of some younger stellar populations present in the periphery, despite the overall older stellar population. No significant tidal features or signs of ongoing major merger events are readily apparent; however, a slight asymmetry or minor disturbance cannot be ruled out without higher resolution data. The overall round shape suggests this is likely an early type galaxy. 
