The galaxy appears as a centrally concentrated system with a smooth, elliptical morphology. The light profile seems to gradually decline from a bright, yellowish core outwards to a greenish-blue halo or disk. It exhibits a moderate degree of ellipticity, appearing somewhat elongated. There is a slight hint of a disturbance or feature in the disk, but it may be subtle and hard to tell from this distance. This system seems to be a galaxy that is not undergoing a major merger, and exhibits a generally well-defined and symmetrical structure, likely representing a relatively relaxed or evolved system.
