This galaxy exhibits a generally smooth morphology, with a predominantly elliptical or spheroidal shape. The light distribution appears concentrated, and there is a significant absence of spiral arm structures. There is some evidence of a possible merger event. There is evidence of two distinct components which are either two galaxies very close to each other, or potentially a single galaxy with a very close companion. It is roughly circular in overall form. Color gradients are present, with the bluer light appearing more prominent in one of the components. The other component emits yellower light. The overall color suggests a galaxy composed primarily of intermediate to older stellar populations, with the blue component indicating a younger stellar population.
