The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish-white hue in the center, potentially indicating an older stellar population. The outer regions of the galaxy appear less concentrated and have a slightly bluer color profile. There are no distinct spiral arms or significant dust lanes visible. The overall structure suggests a galaxy that is well into its evolution, lacking active star formation regions. There is a very slight asymmetry to the galaxy's shape, though no obvious signs of major disturbances or mergers.
