The galaxy presents as a moderately luminous, likely early-type, system with a smooth, elliptical morphology. The core exhibits a concentrated, yellowish hue suggestive of an older stellar population and possibly a supermassive black hole. The galaxy's overall shape is not perfectly circular, displaying a slight elongation. There is a subtle color gradient, shifting towards bluer tones in the outer regions, potentially indicating the presence of younger stars or ongoing, albeit limited, star formation in the outer disk. No strong tidal features or distinct spiral arms are apparent, and the overall structure appears undisturbed, implying the galaxy is not currently undergoing a major merger event.
