The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. It exhibits a gradual decrease in luminosity from the core outwards. There is little discernible dust or distinct spiral arm structure present. The overall color appears to be leaning toward the redder end of the spectrum. It may be undergoing only low levels of star formation. The shape of the galaxy appears to be between round and elliptical, with a slight preference for being in between. There is an appearance of very minimal disturbance to the galaxy, it is likely not undergoing any type of merging event.
