The galaxy presents as a largely smooth, elliptical-type structure with a high degree of central concentration. The core exhibits a bright, concentrated luminosity, likely indicative of a significant stellar population and potentially a supermassive black hole. The overall color is slightly redder, suggesting a population of older stars and a low rate of ongoing star formation. There may be an ongoing merging event with a smaller galaxy, seen by the irregular shape. The merging event is likely minor.
