The galaxy presents as a largely smooth, centralized object with an overall elliptical morphology. The luminosity profile increases sharply towards the galactic center, exhibiting a bright, concentrated core. Moving outwards from the core, the intensity of emitted light gradually diminishes into a faint, diffuse halo. No prominent spiral arms, bars, or distinct features are readily apparent. Slight color variations exist, with the central region tending towards yellow, suggesting the presence of an older stellar population. The peripheral regions show a slightly bluer hue, potentially indicating younger stars, or potentially dust obscuration effects altering the perception of star colors. No signs of ongoing major merger events or significant tidal disturbances are visible.
