The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round with a slight deviation towards an in-between form. The core displays a bright, yellowish-orange hue that gradually transitions to a greenish-yellow halo. This color distribution suggests a stellar population that is evolved, with limited recent star formation activity. There is no visually apparent evidence of spiral arms or disk-like features. The light distribution is fairly even across the visible extent of the galaxy, indicating a lack of significant morphological disturbances or tidal interactions with other galaxies. There is no obvious indication of a major ongoing merger event. The galaxy appears to be isolated.
