The galaxy appears as a single, somewhat amorphous object. Its light profile suggests a relatively smooth distribution, with some hints of deviation from perfect ellipticity. There is a brighter yellow region toward the top, and the lower half appears as a second lobe. There are faint features suggesting it may be undergoing a tidal interaction or a merger event with another galaxy. The color gradients observed, from yellow to red, suggest an older stellar population is prevalent in the core. There appears to be low levels of ongoing star formation. The relatively smooth appearance and general color suggests it is a fairly massive system, possibly a lenticular or early type spiral galaxy.
