The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and centrally concentrated light distribution. The color profile suggests a dominant older stellar population, with a yellowish-red hue. The galaxy shows a high degree of central concentration of light. No spiral arm structures or dust lanes are apparent. The overall morphology indicates a well-mixed and relaxed system. There is little to no indication of on-going significant star formation activity. The galaxy displays no signs of any tidal disturbances or interactions with neighboring galaxies, indicating a dynamically stable system.
