The galaxy appears to be a relatively smooth elliptical galaxy, showing a spheroidal structure with a concentration of older stellar populations towards the center. The color gradient suggests a central bulge region that exhibits a redder hue, possibly indicative of dust obscuration or older, cooler stars. The outer regions seem slightly bluer, which may point to the presence of younger, hotter stars, or a less dusty environment. The overall shape appears mostly circular, with a slight elongation that indicates it is not perfectly spherical. There are no distinct spiral arms or obvious signs of active galactic nuclei in this image. No significant tidal features or indications of recent major merger events are discernible, though subtle asymmetries suggest possible past interactions. The light distribution appears to be diffuse and declines gradually from the core, showing no sharp boundaries.
