The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and concentrated light profile. It has a yellowish hue, suggesting an older stellar population with a lower rate of recent star formation. There is a slight elongation of the galaxy, deviating from a perfect circular shape. Faint, diffuse features are visible in the outer regions, potentially indicating a faint halo. There is a notable lack of spiral arm structures or dust lanes, which further supports the classification as an elliptical galaxy. There is no evidence of any major ongoing merger events or significant tidal disturbances.
