The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-white luminosity, which appears to gradually fade into a diffuse, less luminous halo. The overall color profile suggests a population of older stars. The galaxy's shape is slightly elongated, exhibiting a ratio of axes greater than 2:1, but is not greatly elongated. No prominent spiral arm structures or dust lanes are discernible. There is no noticeable irregular or peculiar morphology, nor are there any clear signs of ongoing merger activity or tidal disturbances. The galaxy’s surface appears smooth, lacking clumpy or knotty structures typically associated with vigorous star formation. Its overall morphology suggests a relatively evolved system, possibly an elliptical or lenticular galaxy nearing quiescence.
