The galaxy presents as a mostly smooth, elliptical-like structure. It exhibits a noticeable central bulge that appears brighter and more concentrated than the surrounding regions. The overall shape is elongated, significantly more cigar shaped than round. There is a subtle suggestion of a disk, though it is not clearly defined. Evidence suggests a non-negligible rate of star formation. No obvious signs of a major ongoing merger are visible, though minor disturbances cannot be ruled out. The color profile is primarily reddish-orange.
