The galaxy appears to be an elongated system, possibly exhibiting a disturbed morphology. The light distribution suggests a primary component that is relatively smooth, with a hint of features or possibly a disk-like structure in the lower region. The galaxy does not appear perfectly round; it has a somewhat cigar-shaped appearance. There are hints of disturbances within the galaxy's structure, potentially indicating minor disturbances or a possible ongoing merger event. The overall color suggests moderate star formation or a mix of stellar populations.