The galaxy presents as a relatively compact system. Its morphology appears largely spheroidal with minimal discernible substructure. The light distribution is centrally concentrated, exhibiting a smooth gradient outwards from the core. There is a slight elongation of the galaxy's shape, though it is mostly round. Its color index, estimated from broad band photometry, suggest an intermediate stellar population mix; the galaxy appears yellowish, indicating neither a very young, blue star-forming population nor a very old, red population. There is no apparent indication of active star formation. No tidal features are discernible, suggesting a relatively quiescent state. The system shows no signs of a major merger event, though some minor disturbances cannot be entirely ruled out. The spatial extent of the object is small and it is most likely a galaxy with a stellar mass around 10^10 solar masses.
