The galaxy exhibits a generally smooth morphology, with a slight elongation suggesting a flattened spheroidal shape. The radial color profile indicates a redder central region, which likely corresponds to an older stellar population. Fainter, bluer regions extend outwards from the core, possibly indicative of areas with more recent, though not intense, star formation. There is a suggestion of some slight disturbance in the morphology, but it is mostly symmetric, appearing not to be significantly influenced by interaction with another object. 
