The galaxy appears as a faint, somewhat diffuse object with a slightly elongated morphology. The light distribution is uneven and shows clumpy features that hint at some internal structure. There is evidence of a possible tidal tail, a structure of stars and gas ejected from the galaxy as a result of gravitational interactions. The overall blue color suggests the presence of at least some young, hot stars, but the general faintness indicates low star formation activity. The galaxy is potentially in the process of merging, as implied by its irregular shape and tidal tail structure.
