The galaxy presents as a system with two primary components. One component displays a largely smooth morphology with a concentrated central region exhibiting a yellowish hue. This suggests a population of older stars. The other component shows a more diffuse, irregular structure with a distinct blue color. This indicates ongoing star formation within this region. There might be signs of tidal disturbances or interactions between the two components, as indicated by the irregular shape of the bluer component. The overall system appears to be relatively small and low in mass. Based on the colors, the rate of star formation might be low. A large fraction of the galaxy is smooth in appearance. The overall shape is neither perfectly round nor highly elongated, suggesting an intermediate stage in its morphological classification. There may be some minor distortions or disturbances present, but the system is not undergoing a major merger event.
