The galaxy appears as an elliptical or lenticular galaxy, exhibiting a smooth and centralized distribution of light. It displays an overall yellow-orange hue, indicative of an older stellar population and a lower rate of on-going star formation activity. The galaxy's shape is more elongated than circular but not extremely so, presenting as moderately elliptical. There's no clear evidence of spiral arm structures or prominent dust lanes. No signs of tidal disturbances or ongoing merger events are visible. The light profile is smooth and concentrated towards the center, suggesting a well-established structure.
