The galaxy presents as a somewhat diffuse object with a discernible, though irregular, morphology. There is evidence of blue light emission in the galaxy indicating the presence of younger, hotter stars, suggesting recent or ongoing star formation. The red component indicates the presence of older stellar populations. There appears to be some form of distortion or tidal feature, which might be due to an interaction with another galaxy. It is difficult to determine whether the morphology is truly a result of a merger without more detailed spectral analysis. The galaxy is small, with moderate brightness. There are indications of slight disturbances present, which could be related to the ongoing star formation or evidence of a minor merger or tidal interaction. The overall appearance suggests an intermediate stage of galaxy evolution, possibly transitioning from a more chaotic, star-forming state to a more quiescent phase.
