The galaxy presents a largely smooth and centrally concentrated morphology. Its overall shape appears nearly circular. The central region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. The galaxy appears to have some faint light extending out beyond the bright core, which fades into the background noise of the image, with no apparent spiral arms or disk-like structures immediately obvious, although a subtle disk cannot be ruled out. There are no obvious signs of ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
