The galaxy appears to be a relatively compact, elliptical or lenticular system. It presents a smooth, centrally concentrated light profile with no discernible spiral arms or prominent disk structure. The central region exhibits a yellowish-orange hue, suggesting a population of older, evolved stars. There's a general lack of blue light which would indicate ongoing, significant star formation within the galaxy, and there is a faint halo. Based on the lack of tidal features or distortions, there appears to be no ongoing major merger activity or significant gravitational interaction with nearby galaxies.
