The galaxy presents as a slightly elliptical, lenticular structure with a smooth, mostly featureless profile. The light distribution appears relatively concentrated, with the highest intensity emanating from the central region. The color index suggests a bias toward redder wavelengths, indicative of an older stellar population and/or significant dust obscuration. There may be a faint hint of disturbed morphology, such as a possible tidal feature, but the image resolution makes a definitive assessment challenging. There is a close pair of brighter sources slightly offset from the galaxy's main body, which may either be related to the galaxy or be chance alignments. This object appears to be a massive, relatively evolved galaxy undergoing low levels of star formation.
