The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, indicating a high stellar density and/or active galactic nucleus. The light profile smoothly decreases outward from the core, with no distinct spiral arm structures or significant dust lanes apparent. The color appears to be predominantly yellow-red, suggesting an older stellar population with fewer young, massive blue stars. There is no apparent merger activity or significant tidal disturbances. The galaxy's structure is predominantly spheroidal, with little indication of a flattened disk component.
