The galaxy presents as a singular, centrally concentrated light source. The light emitted is a general yellow to orange hue, suggestive of an older stellar population. The object appears relatively smooth in texture, with no clear signs of spiral arms or a bar structure. The galaxy could be generally classified as an elliptical galaxy or a lenticular galaxy observed at a substantial distance. Based on the concentration of light, it does not seem to be undergoing major mergers. There may be another source nearby, perhaps gravitationally bound to it.
