The galaxy presents as a slightly elongated, elliptical form with a smooth, concentrated light distribution. The core exhibits a bright, yellowish-white luminosity that gradually fades outwards, displaying a yellow-orange hue. The galaxy shows no distinct spiral arm structures or obvious dust lane features in this imaging, suggesting a relatively evolved stellar population. There is a subtle indication of a faint, extended halo, but the overall structure is dominated by its spheroidal central bulge. There are no indications of any merging or tidal disruptions present.
