The galaxy presents as a well-defined, elliptical morphology with a smooth, featureless appearance. The light profile gradually diminishes from the center outwards, exhibiting no prominent spiral arms or bar structures. The galaxy's color index suggests a population of older stars, dominated by redder wavelengths. There is a lack of observable dust lanes or regions of active star formation within the galaxy's disk. The overall shape indicates an oblate spheroid, but the galaxy appears to be oriented almost face-on from our vantage point. There is no visible evidence of tidal disturbances or interactions with nearby galaxies, suggesting it is relatively undisturbed.
