The galaxy appears as a single, relatively smooth and elliptical structure. There is a slight elongation, but it is mostly rounded. The galaxy exhibits a yellowish hue, suggesting a population of older stars with lower star formation rate. The light distribution suggests a significant central concentration. There appears to be an interacting galaxy or a significantly disturbed region to the south of the main body. It presents as a separate, but closely associated, point of light, somewhat smaller and rounder, with slightly more pronounced yellow tone. The galaxy likely exhibits an estimated stellar mass on the order of 10^10 to 10^11 solar masses.
