The galaxy presents as a centrally concentrated object with a largely smooth, featureless morphology. It exhibits a roughly elliptical shape, appearing nearly round. The core region displays a bright, yellowish-white luminosity, suggestive of an older stellar population. Moving outward from the core, the galaxy shows a gradual decrease in brightness and a transition to a slightly bluer hue in the outer regions. There is a subtle suggestion of a disk-like structure, but without prominent spiral arms. The overall structure indicates a relatively evolved system, likely an early-type galaxy or a spiral galaxy with a dominant bulge. Evidence suggests a low star formation rate and a high mass. There may be a hint of a minor disturbance in the galaxy's structure. 
