The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A pronounced central bulge is observed, exhibiting a yellowish-orange hue, suggesting a population of older stars. The overall structure appears largely featureless, with no apparent spiral arms or dust lanes visible. The galaxy's light profile decreases gradually from the core outwards, indicative of a well-established stellar population. Minor asymmetries or disturbances are not obviously present, and the galaxy appears relatively undisturbed in terms of its overall shape.
