The galaxy presents an overall elliptical morphology, displaying a moderate degree of central concentration. It is likely a lenticular galaxy. The light distribution appears relatively smooth, with no prominent spiral arm structures visible in this image. The color profile suggests a population of older stars, contributing to the galaxy's yellowish-white hue. The galaxy has a secondary object or core to the northwest. The galaxy shows signs of gravitational disturbance, appearing to be slightly warped or elongated and possibly merging with another galaxy.
