The galaxy appears to be a relatively smooth, elliptical system. It presents as a concentrated spheroid of light, exhibiting a gradual decrease in luminosity from the core outwards. There's a subtle color gradient, with the central region exhibiting a slightly yellower hue that transitions to a bluer tone in the outer regions of the galaxy. There is little visible evidence of significant spiral arm structure or active star formation regions. The galaxy exhibits a regular morphology, with no obvious signs of tidal disturbances or ongoing merger activity.
