This galaxy exhibits a somewhat smooth morphology with a hint of disk-like structure. The color gradients suggest a mix of stellar populations. A central concentration of older, redder stars appears prominent, with a surrounding, slightly flattened distribution of younger, bluer stars. There is evidence of an ongoing or recent interaction or merger event. Multiple distinct components are observed, including what may be a central bulge or nucleus. Tidal tails and/or faint plumes are present. The dominant shape is somewhat rounded, but it deviates significantly from perfect circularity.