The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated bulge with a noticeable decrease in luminosity as it extends outward. There is very little evidence of spiral arms, bar structures, or significant dust lanes, which supports its classification as elliptical. The overall color is a somewhat even, with a slight redder hue in the central region that transitions to a bluer tinge on the outer fringes. The redder core might indicate a population of older, cooler stars. The blue outer colorations, although faint, hint at some ongoing, although subdued, star formation within the galactic periphery. The disk appears to have minimal signs of tidal disruption or interaction with other galaxies. Its rounded shape also gives it the appearence of being a relatively relaxed system.
