The galaxy presents as a somewhat elongated, disk-like structure. It appears to be relatively smooth in overall texture, with a high degree of central concentration. A distinct color gradient is observed, transitioning from a reddish hue in the central region to a bluer tint at the outer edges. The overall shape suggests the galaxy is neither perfectly circular nor highly elongated, and that it is likely an elliptical galaxy with a slight disk-like morphology. There is no obvious evidence of strong tidal disturbances or ongoing major mergers. The galaxy appears relatively undisturbed and isolated.
