The galaxy presents a generally smooth, elliptical morphology. It exhibits a slightly elongated shape, with the major axis oriented approximately vertically. The light distribution appears centrally concentrated, with a gradual decrease in intensity outward from the core. There are no prominent spiral arms or a distinct disk component visible in this image, suggesting a relatively old stellar population with little ongoing star formation. There is a faint blue-ish hue to the galaxy, as if star formation may have recently been present, and the galaxy does not appear to be undergoing any major merging events. The morphology appears relatively undisturbed.
