The galaxy appears to be a relatively smooth and featureless system. Its overall shape is elliptical, with a noticeable elongation along one axis, creating a cigar-like appearance. There is a subtle color gradient from the central region outwards, with the core exhibiting slightly bluer hues, potentially indicating the presence of younger stellar populations or ongoing star formation, however its star formation rate and specific star formation rate are low. The galaxy does not show any signs of major disturbances or mergers and appears to be relatively isolated, without any nearby interacting companions. The color indices suggest it may consist predominantly of evolved stars and an older stellar population.