The galaxy presents a generally smooth appearance, with a slight elongation, suggesting a possible elliptical morphology or a disk galaxy seen at a significant inclination. Its color is generally redder than some of the foreground objects, indicating an older stellar population or significant dust obscuration. There is no strong evidence of spiral arm structure or active star formation regions visible in this image. The overall structure appears relatively undisturbed, showing no strong indications of ongoing major mergers or significant tidal interactions with nearby galaxies. There might be a minor dust lane bisecting the galaxy, but more resolution is needed to tell.
