This galaxy exhibits a generally smooth morphology, appearing largely spheroidal in shape. The galaxy’s light is concentrated in a central region with two distinct bright yellow cores, suggesting a possible ongoing or recent merger. Peripheral to the bright center, a more diffuse, lower-intensity halo or extended envelope of stellar material can be observed. There is some indication of disturbances in the galaxy's overall shape beyond the very center, hinting that the merging process may still be affecting its structure. Overall color indices indicate it is primarily comprised of older stars, although the relative yellowness of the core may indicate the presence of more recent star formation.
