The galaxy presents a morphology suggestive of an ongoing or recent merger. Two distinct, roughly spheroidal luminous components are visible, both exhibiting a yellowish hue. The object's overall shape appears elongated, oriented along a roughly horizontal axis. The relative size of the system suggests an intermediate-mass galaxy. There is a hint of faint tidal features, such as streams or tails, suggesting a relatively recent interaction. The luminosity and color index suggest the object is composed of relatively old stellar populations, indicating that star formation is occurring at a low rate.
