The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. Its overall shape is generally round. The color profile suggests a population of older stars, indicated by the reddish-yellow hue of the central bulge. The presence of some subtle disturbances and asymmetries in the outer regions may suggest a possible ongoing or recent interaction with another galaxy, though a merging event is not definitive from the image. There's a hint of a disk shape, but the smooth fraction dominates.
