The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light profile. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions appear more diffuse and slightly bluer in color, possibly indicating the presence of a younger, albeit less prominent, stellar component. The overall shape is nearly circular, displaying minimal deviation from a perfect ellipse. No prominent features like spiral arms, dust lanes, or tidal tails are apparent. There is no evidence of ongoing major merger activity, although some minor disturbance cannot be ruled out. The object's small apparent size indicates that it is at a significant distance.
