The galaxy presents a slightly elongated, somewhat amorphous structure. Its central region appears brighter and more concentrated, with the light gradually fading towards the edges. The overall color is a warm hue, suggesting a significant population of older stars, but there may be some faint blue regions, which would indicate the presence of younger, hotter stars. There isn't any distinct spiral arm structure and the galaxy is fairly smooth in appearance with some subtle disturbances, not indicative of an ongoing major merger. 
