The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. A slight elongation is discernible, deviating marginally from a perfectly circular shape. Color gradients suggest a higher concentration of older stellar populations in the core, indicated by the yellowish-white hue, transitioning to a bluer tint in the surrounding halo. Subtle irregularities in the outer regions may indicate minor tidal interactions or past merger events. The galaxy is relatively undisturbed, with no prominent spiral arms or significant dust lanes visible.
