The galaxy appears as a relatively smooth, elliptical structure. Its color gradient transitions from a reddish-orange central bulge to a bluish-white outer region, indicating a mix of older and younger stellar populations. The galaxy exhibits an elongated shape, not perfectly spherical but also not highly flattened into a disk. There are no obvious signs of spiral arms or prominent dust lanes. Some minor asymmetry or perturbation in the outer regions might suggest a possible minor interaction with another galaxy or past merger event, but the overall morphology suggests it is generally undisturbed.
