The galaxy appears to be a relatively smooth, elliptical type. It exhibits a central bulge that appears bright and concentrated. The overall shape is elongated, with a cigar-like form rather than being perfectly spherical. There is a slight indication of a disk or some features beyond the smooth light distribution, and there is no obvious sign of merging activity or major disturbances. The color is somewhat red, hinting at an older stellar population and low levels of ongoing star formation within the galaxy. The light gradually fades from the center to the outskirts.
