The galaxy appears as a centrally concentrated object with a relatively smooth morphology, exhibiting a yellowish-orange hue. The light distribution suggests a high degree of radial symmetry with no obvious spiral arm structures or a prominent disk. It is a relatively compact galaxy of medium size. There may be some minor disturbances or a possible tidal tail visible suggesting a recent interaction or merger. Overall, the galaxy exhibits characteristics of a relatively evolved system with potentially suppressed star formation activity.
