The galaxy presents a largely smooth morphology, appearing as an elliptical or lenticular galaxy. It exhibits a relatively round shape, lacking any pronounced disk or spiral arm features. There's a slight indication of tidal disturbance, however, the bulk of the object is round and consistent with an older system of stars. The color index suggests a population of older stars dominating the galaxy's light output. This is consistent with the smooth morphology and lack of distinct features such as spiral arms, suggesting that star formation is either minimal or has largely ceased. The overall structure doesn't indicate any ongoing major merger activity, further supporting the hypothesis that the galaxy is a relatively settled, evolved system.
