The galaxy appears to be a relatively smooth, elliptical-like structure. A bright central bulge dominates the core, showing a gradual decrease in intensity towards the outer regions. The color gradient suggests older stellar populations concentrated within the core, shifting towards slightly bluer tones in the surrounding areas. There's no obvious spiral arm structure, but a faint hint of a disk-like component might be present in the extended regions. Overall, the galaxy appears to be a fairly regular system with a lack of significant disturbances or ongoing major merger activity.
