The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile with a gradual decrease in intensity outwards from the core. The core appears golden and luminous, transitioning to redder hues in the outer regions. There is no distinct spiral arm structure or obvious dust lane obscuration visible, suggesting a relatively evolved system. The lack of pronounced features indicates a well-mixed stellar population. The overall shape appears roughly circular but is slightly elongated. There is no obvious evidence of active galactic nuclei activity within the limits of the image's resolution. There are no major disturbances or mergers apparent, the galaxy is quite uniform.
