The galaxy presents a generally smooth morphology, with a notable absence of well-defined spiral arms or a prominent central bulge. The light distribution is relatively even, though it appears to be undergoing a significant merger. The object exhibits a moderate red-shift suggesting it is a relatively distant object. There appear to be no distinct dust lanes or knots of star formation visible within the galaxy's structure at this resolution. The light appears to be distributed into two distinct blobs. This is likely a major ongoing merger. There may be some tidal tails, although this is not clear from the resolution. Overall, the galaxy appears to be in a relatively advanced stage of development.
