The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. There is an absence of spiral arm structure, which, along with its round shape, is consistent with an elliptical morphology. The light distribution is centrally concentrated, with the brightness decreasing smoothly from the center outwards. The galaxy exhibits a reddish-orange hue, suggestive of an older stellar population and low levels of current star formation. There is some evidence of possible tidal disturbances or interactions, with faint, diffuse extensions emanating from the main body. The color suggests that it is a relatively massive galaxy that is not forming many stars. It is possible that we are seeing an ongoing merger event, or some past disturbance that altered its morphology.
