The galaxy presents a generally smooth, elliptical morphology. It appears relatively compact, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. A fainter, slightly bluer halo surrounds the core, indicating the presence of a more distributed population of younger stars. There is indication of potential disturbance to the morphology of the galaxy, perhaps due to a potential merger event in its past or currently occuring.
