The galaxy appears to be a relatively compact, elliptical system, with a smooth and concentrated light profile. The central region exhibits a yellowish-white hue, suggesting an older stellar population. There are no distinct spiral arm structures or significant dust lanes visible. The overall shape is generally round, with only a slight deviation towards an elongated form. Evidence of ongoing or recent major merger activity is not apparent. Faint, diffuse light extends outwards from the core, indicating a surrounding stellar halo, however it appears relatively faint and indistinct. There is a faint blueish hue surrounding the yellow-white core, indicative of some younger stars that contribute to its overall color.
