The galaxy exhibits a morphology that is predominantly smooth in appearance. While it displays some degree of structure, the smooth component dominates the overall visual impression. It appears somewhat elliptical, with an intermediate roundness. There is no substantial evidence of a major merger, although it could be experiencing minor disturbances, perhaps internal or due to minor interactions. The overall color suggests a evolved stellar population, with a higher concentration of older, redder stars compared to younger, bluer ones. It shows a reduced rate of star formation. Its relatively large size indicates a significant stellar mass.
