The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright with a yellow-orange hue. Moving outwards from the core, the luminosity gradually decreases, with no discernible spiral arm structures or distinct features readily apparent. The outer regions suggest a somewhat flattened shape, deviating slightly from a perfectly circular profile. There are no signs of significant tidal disturbances or ongoing major mergers. The overall color suggests an older stellar population, potentially with suppressed levels of ongoing star formation. The galaxy displays a relatively compact size, with a well-defined edge that fades into the background sky.
