The galaxy appears as a centrally concentrated, relatively smooth object. The light distribution suggests a spheroidal morphology, possibly an elliptical galaxy or a lenticular galaxy seen face-on. There's a slight elongation, but it's nearly round in projection. The color is primarily a yellow-orange hue, indicating an older stellar population, and suggesting relatively low ongoing star formation. There is very faint bluer emission in its outer regions, which might mean there's a minor disk structure in the outer parts, or it could be the result of image artifacting. There is no obvious presence of spiral arms or strong dust lanes from what is visible. There are no major signs of an ongoing merger, but there may be a slight asymmetry, suggesting a minor interaction in the past.
