The observed galaxy presents an asymmetrical morphology. It is likely a spiral, though this is difficult to assert due to its irregular form. At the center there is a bright nucleus, which is surrounded by a relatively bright and uniform inner disk. Radially outward from the nucleus, there are hints of what may be some form of outer disk. These outer arms are very faint and difficult to clearly identify. There seems to be at least one tidal tail feature extending from one side of the outer disk, which may indicate recent gravitational interaction. The galaxy appears relatively blue, indicating the presence of hot, young stars. This may point to ongoing star formation activity within the galaxy, perhaps triggered by a past or ongoing merger event.
