The galaxy presents an elongated, oval morphology. It appears to be a disk galaxy, potentially viewed close to edge-on. There is a noticeable central bulge region that is brighter and more concentrated. Faint, diffuse light emanates from the disk, with hints of structure suggesting the presence of spiral arms, though these are not clearly defined. The overall color is bluish, which hints at the presence of a younger, hotter stellar population. The galaxy doesn't appear to be undergoing any major mergers or significant tidal disturbances, and its structure seems generally undisturbed, though there may be some minor asymmetry present.
