The galaxy presents as a moderately bright, elongated elliptical form. Its central region appears brighter and more concentrated, displaying a yellowish hue, potentially indicating an older stellar population. The outer regions exhibit a smoother, less defined structure with a bluer tint, possibly indicative of ongoing star formation. There is no discernible spiral arm structure. The galaxy appears relatively undisturbed with no obvious signs of merging or major tidal interactions. Its overall shape suggests it lies somewhere between a perfectly round and an elongated form.
