The galaxy presents as a generally smooth, elliptical structure, exhibiting a moderately elongated form. The color profile suggests a dominant population of older stars, manifesting as a yellowish-orange hue concentrated towards the galactic center, with relatively little presence of bluer, younger stars. The light distribution is fairly uniform, lacking significant spiral arm structures or distinct star-forming regions. There is no obvious presence of a prominent dust lane or other obscuring material within the galaxy's structure, and there are no readily apparent signs of tidal disturbances or ongoing mergers with other galactic bodies. The overall appearance indicates a galaxy undergoing relatively low star formation and possessing a high degree of morphological stability.
