The galaxy presents as a somewhat elongated elliptical shape, exhibiting a smooth, diffuse light distribution. A brighter central region is apparent, suggesting a concentration of stars and possibly a supermassive black hole at the galactic nucleus. The light appears relatively uniform, with no obvious spiral arms or distinct features. The overall color seems slightly blue-ish/white, which may indicate a moderate level of ongoing star formation, but this interpretation warrants further investigation based on color indices. The galaxy exhibits a noticeable tilt relative to our line of sight and has an estimated effective radius of approximately 2 kpc. Based on its morphology, the galaxy is likely an early-type galaxy, possibly of the S0 or elliptical type. There is no obvious evidence of any major mergers or significant tidal disturbances within this image.