The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. The core region exhibits a bright, yellowish hue, suggestive of a population of older stars. The outer regions display a gradual decline in luminosity, fading into the background sky. There is a subtle elongation in the morphology. The smoothness of the light profile indicates a lack of significant spiral arm structures or prominent dust lanes. The overall appearance is consistent with an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy is relatively isolated, with no immediately apparent signs of tidal interactions or recent merger events.
