The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration, with a bright, unresolved core suggestive of a significant bulge component. The galaxy appears largely featureless, lacking prominent spiral arms or dust lanes. The color gradient indicates a population of older stars, potentially with ongoing low levels of star formation. There is no evidence of any recent major merger events, although there might be some sign of tidal disturbances nearby. The overall shape is spheroidal and appears fairly relaxed.
