The galaxy presents as a singular, relatively smooth structure. It exhibits a generally elliptical morphology, appearing mostly rounded in shape. A color gradient is visible, with a yellowish-white core transitioning to redder hues towards the outer edges. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. There are no obvious signs of major mergers or tidal disturbances, though subtle, minor disturbances cannot be entirely ruled out. The galaxy appears to be a fairly isolated system within the observed field.
