The galaxy presents as an elliptical system, exhibiting a smooth, relatively featureless morphology. There is a centrally concentrated bulge that appears to be composed primarily of older stars, indicated by the yellowish-orange hue. The galaxy appears moderately luminous, with a smoothly declining radial profile. There are no obvious spiral arms or dust lanes. The isophotes are generally elliptical, with a moderate ellipticity; it is neither perfectly spherical nor highly elongated. There are no signs of major tidal disturbances, mergers, or significant star-forming regions that would typically be visible as blue knots within the galaxy. The galaxy appears as an isolated object, as no other objects are gravitationally bound.
