The galaxy presents as a single, relatively smooth object, dominated by a bright central region. The light distribution is highly concentrated, fading gently outwards. A hint of a disk may be present, but the object is dominated by its bulge and appears spheroidal. The galaxy exhibits a yellowish-red hue, suggestive of an older stellar population. There is no visible evidence of spiral arms or significant dust lanes. The galaxy appears to be in a relatively quiescent state with a very low star formation rate. There are no obvious signs of recent or ongoing mergers. The galaxy's high degree of roundness suggests it is likely an elliptical galaxy or a lenticular galaxy seen face-on.
