The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a flattened, disk-like structure, viewed at an oblique angle. The central bulge appears bright and concentrated, gradually fading into the outer regions. There is a subtle color gradient, transitioning from a yellowish-white core to a bluer hue in the surrounding disk, which may indicate ongoing, but minimal, star formation. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or major mergers. Minor disturbances cannot be ruled out at this resolution. The overall shape is predominantly in-between round and elongated. The light distribution is regular and without obvious irregularities.
