The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a near-spherical shape, with only slight deviations from perfect circularity. The light distribution is relatively even across the galaxy's body, indicative of a well-mixed stellar population. There is no evidence of strong spiral arm structures or a prominent disk. Faint hints of asymmetry might be present, suggesting a possible past interaction or minor disturbance. The overall color profile suggests a mature stellar population, with a relatively low ongoing star formation rate, but is still actively forming stars. No clear signs of a major merger event are evident, although subtle disturbances may exist.