The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is somewhat elongated, but tending towards round. The core region exhibits a bright, concentrated luminosity, possibly indicating a significant concentration of older stars or perhaps even activity from a supermassive black hole. There appears to be a slight color gradient visible, with the central region appearing bluer and the outer regions showing a slightly redder hue. There is a noticeable lack of prominent spiral arms or distinct dust lanes. The galaxy does not appear to be undergoing any major merging activity, though minor tidal disturbances cannot be ruled out. 
