The galaxy appears as a centrally concentrated object with a fairly smooth profile. There is little evidence of spiral arms or a prominent disk structure; the morphology is more indicative of an elliptical or lenticular galaxy. Its light profile suggests a relatively homogenous stellar population. The color is slightly bluer than a typical elliptical galaxy suggesting some on-going star formation but that star formation rate is likely to be relatively low. There is also an absence of any obvious tidal features or signs of a major merger event, but there may be minor disturbances present.
