The galaxy appears to be a relatively smooth, elliptical-type galaxy, potentially exhibiting some minor disturbances. It is characterized by a high degree of roundness and a lack of distinct spiral arms or a prominent disk structure. The light is more concentrated in the center of the galaxy. The galaxy seems to have a reddish hue, suggestive of an older stellar population and a relatively low rate of current star formation. There is a second, less-defined galaxy nearby. There are no obvious signs of a major ongoing merger event, although some minor interaction might be possible, given the disturbance and nearby galaxy.
