The galaxy appears as a centrally concentrated object with a predominantly smooth morphology. There is only a vague impression of a disk structure; this might represent a spiral galaxy with tightly wound arms or a lenticular galaxy. The central bulge appears to be a significant component. The overall color of the galaxy appears to be a pale yellow, possibly indicating an older stellar population with relatively low levels of on-going star formation. There appears to be no sign of any major merger events, although the hint of a disk structure might indicate that the galaxy experienced a minor disturbance at some point. There may be some slight asymmetry in the outer regions of the galaxy, but the overall shape is fairly regular.
