The galaxy appears to be a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge with a decrease in luminosity moving outwards. The core of the galaxy presents a slightly reddish hue, possibly indicative of an older stellar population. The surrounding halo appears slightly bluer, suggesting the presence of younger stars, though this is not very pronounced. The galaxy does not exhibit any apparent spiral arm structures or signs of major disturbances or mergers. The overall morphology suggests a mature, relatively undisturbed system. The shape is mostly round, without elongation into a disc-like structure.
