The galaxy presents as a relatively smooth, elliptical-like object with an intermediate axial ratio. The central region exhibits a concentrated, bright core, appearing yellowish in color, likely indicating an older stellar population. This suggests a lack of significant ongoing star formation within the nuclear region. Extending outward from the core, the galaxy shows a gradual decrease in surface brightness. While subtle, there are hints of a disk-like structure. There is some subtle blue scattered throughout, possibly pointing to a small amount of younger stars throughout the disk of this galaxy. No spiral arm structure is evident from the image. No obvious signs of tidal disturbances or major merger activity are seen.