The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a somewhat elongated, cigar-shaped morphology. The light distribution suggests a central bulge that is bright and concentrated. The overall color is slightly reddish-orange, possibly indicating an older stellar population with reduced star formation activity. There are subtle hints of bluer regions along the outer edges which may indicate low-level star formation. Evidence suggests that it is not currently undergoing a major merger, though the slight distortion to its morphology suggests it may have been involved in a minor disturbance.
