The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The core exhibits a yellow-white hue, suggesting a population of older stars dominating the central regions. Fainter, bluer emissions extend outward from the core, hinting at the presence of younger stars or ongoing star formation in the surrounding regions. The galaxy does not present a distinct spiral structure or prominent disk features. It seems to be an elliptical galaxy. The overall shape is approximately circular, with a slight elongation along one axis. No significant tidal features or signs of recent mergers are readily apparent. The light is consistent with a relatively quiescent galaxy with a low star formation rate.
