The galaxy presents a largely smooth morphology with a subtle, extended structure. It exhibits a central concentration of light that gradually diffuses outwards. The shape appears to be somewhere between elliptical and lenticular, being not perfectly round but not displaying prominent spiral arm features. The color profile suggests a relatively older stellar population, but hints of bluer regions suggests on-going low levels of star formation. There is some indication of minor disturbances or faint tidal features, suggesting a possible past interaction or merger event, although the overall structure is largely undisturbed.
