The galaxy appears as a single, largely featureless entity. It exhibits a smooth morphology with a generally elliptical shape, appearing almost perfectly round. The light profile suggests a centrally concentrated structure, with a gradual decrease in intensity moving outward from the core. The core region displays a warmer, yellowish-orange hue. Fainter greenish light is present in the surrounding area, possibly indicating older stellar populations or differing chemical compositions. No distinct spiral arms or dust lanes are readily apparent, suggesting a possible lack of significant ongoing star formation. There are no signs of any major mergers or tidal disturbances.