The galaxy presents a primarily smooth morphology, with a dominant central bulge exhibiting a yellow-orange hue. This suggests a population of older stars, likely with relatively low ongoing star formation. The galaxy appears largely spheroidal, with a high degree of roundness. There is a hint of a possible minor disturbance or feature, and the galaxy does not appear to be undergoing any major merger activity. The overall structure indicates the galaxy may be classified as an elliptical galaxy.
