The galaxy appears to be a spiral galaxy, viewed at a moderate inclination. There are tightly wound spiral arms which are relatively smooth and exhibit distinct blue color, suggesting active star formation within them. The arms emerge from a central bulge, which appears moderately sized. The galaxy exhibits a weak bar structure spanning the central region. There is no obvious evidence of major mergers or significant tidal disturbances affecting the overall structure. The galaxy disk appears relatively undisturbed, and the overall appearance suggests a system undergoing relatively normal spiral evolution. The absence of intense red hues suggests a comparatively low abundance of older stellar populations, and the blue color across a large portion of the disk suggests that the star formation is active.
