The galaxy appears to be a relatively smooth, elliptical or lenticular system, exhibiting a centrally concentrated morphology. The primary light distribution is fairly uniform, suggesting an older stellar population with little ongoing star formation. There is a slight elongation or flattening, but overall, it appears nearly round in projection. Evidence of a possible minor interaction or disturbance cannot be ruled out due to a possible slight asymmetry. It is likely a massive galaxy, emitting strongly in the green, red, and z-bands. The object is potentially in the process of merging with another galaxy, but additional data is required.
