The galaxy presents as a centrally concentrated, smooth light distribution, likely an elliptical morphology. The object exhibits a general yellowish-white hue, with a brighter core. There is very little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a relatively old stellar population, as well as a very low star formation rate, which aligns with what would be expected from an elliptical galaxy. The elliptical appearance of the galaxy suggests a relatively round shape when viewed from our perspective.
