The galaxy presents as a somewhat elliptical, disk-shaped object with a smooth, diffuse appearance. The central region exhibits a concentration of light, appearing yellowish-orange in color, potentially indicating an older stellar population and minimal ongoing star formation in the core. The outer regions of the galaxy show a bluer tint, suggestive of younger stars. There are no apparent distinct spiral arm structures or significant dust lanes visible, although some minor irregularities are present. Overall the galaxy appears undisturbed, showing no signs of major merger activity.
