The galaxy presents as a smooth, elliptical structure. The central region is characterized by a bright, concentrated core, exhibiting a yellowish hue, suggesting a population of older stars. The outer regions display a gradient transition toward bluer colors, potentially indicative of ongoing or recent star formation activity within a disk-like structure. The galaxy exhibits a slight elongation, neither perfectly circular nor highly elongated. There is no obvious indication of major tidal disturbance or a recent merger, the galaxy shows high levels of smoothness. No spiral arm structures are visible within this image. 
