The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears largely smooth and elliptical, with a notable lack of discernible spiral arms or significant substructure within the main body of the galaxy. The color gradient suggests a moderate population of older stars, with the core region exhibiting a slightly yellower hue. Based on the absence of clear tidal features or asymmetries, the galaxy does not appear to be undergoing any major ongoing merger events or significant gravitational disturbance. There may be minor irregularities, but overall it presents as a fairly relaxed system.
