The galaxy presents as a fairly elliptical, smooth object. Its core is a bright, concentrated central bulge, indicating a high stellar density. The luminosity fades gradually from the core outwards, suggesting a lack of distinct spiral arms or other prominent structural features. The color appears to be yellowish, which could indicate an older stellar population. There appears to be very little dust and gas content within the galaxy. The overall morphology suggests that it is likely an elliptical galaxy with an estimated diameter of around 4.5 kpc, and is approximately 13% redshifted. This implies the object is relatively massive and possesses a mass greater than 10^10 solar masses. There is little evidence of ongoing or recent major mergers or interactions. The object is likely not forming many new stars.