The galaxy presents a flattened, elliptical morphology. A bright, concentrated nucleus dominates the central region, exhibiting a smooth, featureless appearance. The luminosity decreases steadily from the core outwards, transitioning into a more diffuse, elongated halo. There's a slight hint of a disk structure, but it is not well defined. Some subtle, disturbed features indicate a possible interaction or minor disturbance, though no clear signs of a major ongoing merger are obvious. There is a very faint dusty ring that can be seen, but is very difficult to make out without additional magnification. The color appears relatively uniform across the galaxy, with a general trend towards redder hues, suggesting an older stellar population and a lower rate of ongoing star formation.
