The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge that appears yellowish in color. The galaxy's light profile appears to gradually fade from the core, suggesting a well-established stellar population. A slight bluer coloration is apparent at one end of the galaxy, and a slight disk may be present. There is no obvious tidal debris or strong visual evidence of recent major merger activity, though minor disturbances cannot be ruled out. The galaxy's apparent angular size is relatively small, which suggests a considerable distance given it's magnitude. The overall appearance points toward a galaxy that is either an elliptical galaxy or a spiral galaxy with a dominant bulge and little star formation.
