The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is somewhat elliptical, elongated more along one axis, but not significantly cigar-shaped. There is a bright, unresolved core region, suggesting a high concentration of stars or a possible active galactic nucleus, although it's difficult to confirm from this image alone. The surrounding disk or bulge component exhibits a gradient in color, with the central region appearing bluer, possibly indicating more recent or ongoing star formation relative to the outer regions, which appear redder. There is little evidence of strong spiral arm structure or significant dust lanes from this image. Faint, diffuse light extends from the central regions. The galaxy does not appear to be strongly interacting or undergoing a major merger, though there might be some minor disturbances or asymmetries, particularly in the faint outer regions, suggesting past interactions or minor mergers.
