The galaxy appears as a single, relatively smooth object with a slightly elongated, round shape. Its color suggests an older stellar population, exhibiting a yellowish-red hue, indicative of evolved stars dominating the light output. There is no discernable presence of spiral arms or a prominent disk structure. A central, brighter region might indicate the presence of a galactic bulge or a supermassive black hole. There are no obvious signs of recent mergers or significant tidal disturbances, although a slight asymmetry in the outer regions cannot be ruled out with complete certainty.
