The galaxy presents as a somewhat amorphous, though predominantly smooth, structure. Its light profile suggests a centrally concentrated core that is less prominent than the extended halo surrounding it. There are no distinct spiral arms or bar structures visible, and the overall shape appears more elliptical than disk-like. There is also a faint tidal disturbance, which is evidence that this galaxy has been interacting with another galaxy. The galaxy exhibits a generally blue hue. The galaxy appears to be moderately massive, and has a low rate of star formation.
