The galaxy presents as a single, relatively smooth object with an elliptical morphology. There appears to be a concentration of light towards the center, suggesting the presence of a prominent bulge. The galaxy exhibits a somewhat round shape, with a gradual decrease in light intensity from the core outwards. Faint traces of what may be a disk-like structure are visible in the outer regions, however they are very faint. Overall, the galaxy shows no signs of major disturbances or ongoing mergers, and appears relatively undisturbed.
