The galaxy presents as a single, relatively smooth, and centrally concentrated structure. It exhibits an elliptical morphology and golden hue. While some asymmetry is present, no distinct spiral arms or a prominent disk are discernible at this resolution. It is unclear if the features are being obscured by dust, but some irregularities hint at a possible interaction or merger event. The galaxy appears somewhat compact with a small angular size. There are no tidal tails or extended halos visible in this image. It is plausible that the central concentration of light indicates a significant bulge component, characteristic of a galaxy nearing the end of its star-forming epoch.
