The object appears to be a galaxy at a considerable distance, evidenced by its small angular size. It exhibits a smooth, elliptical morphology with a high degree of central concentration. The color profile suggests an older stellar population, with a dominant red-yellow hue in the central bulge. A faint blue tinge around the edges may indicate some ongoing, but limited, star formation in the outer regions. There are no readily apparent spiral arms or other distinct features. No signs of any major disturbances due to a recent merger. The overall impression is that of a relatively evolved system with minimal current activity.
