The galaxy appears as a centrally concentrated, relatively smooth elliptical. Its color profile suggests an older stellar population, with a yellow-red hue dominating the core and outer regions. It exhibits a high degree of roundness, showing minimal deviation from a circular shape. There are no clear signs of spiral arm structure or a prominent disk. It is not entirely homogenous and has a slight amount of structure. It appears that there is no ongoing major merging activity, but the galaxy could be interacting or have interacted with another smaller galaxy at some point. Its size is moderate, with its light extending over a limited angular extent. 
