The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. Its color profile indicates a dominant population of older stars, evidenced by the redder hue concentrated toward the galactic center, with slightly bluer regions in the outer areas of the galaxy. It demonstrates a high degree of central concentration, with the luminosity decreasing smoothly from the core outwards. There is little evidence of spiral arms or a prominent disk structure. There are possible tidal features or minor disturbances located at a lower declination from the primary mass of the galaxy. The overall color and morphology suggest an evolved system, likely with a relatively low star formation rate and a significant stellar mass.
