The galaxy appears to be a spiral galaxy, characterized by a central bulge and a disk. The bulge is relatively prominent and appears roughly spherical, with a bright, concentrated core indicative of a high stellar density. Faint spiral arms extend outward from the bulge, though they are not sharply defined and appear somewhat diffuse. The disk shows a bluer color than the bulge, suggesting a younger stellar population and ongoing star formation. The overall structure suggests a relatively undisturbed galaxy, with no obvious signs of major mergers or tidal disruptions, though there is a suggestion of minor disturbances within the spiral arm structure. The galaxy's morphology appears intermediate between a pure bulge and a more clearly defined spiral disk, presenting a transition in stellar populations and structure.
