The galaxy presents a generally smooth and rounded morphology. There is a prominent central bulge that appears to be a relatively old stellar population, indicated by its yellowish-white hue. The outer regions exhibit a fainter, more diffuse glow, possibly indicating the presence of a stellar halo or a less concentrated disk component. There is no obvious spiral structure or distinct dust lanes visible, suggesting it is likely an elliptical or lenticular galaxy. Minor asymmetry can be observed; the galaxy is more extended in one direction, though no major disturbances or merging features are apparent.
