This galaxy presents as a grand design spiral, exhibiting well-defined arms that emanate from a central bulge. The spiral arms appear relatively tightly wound in the inner regions, becoming more open as they extend outwards. The bulge component has a yellowish color, indicating an older stellar population, while the spiral arms display a bluer hue, suggestive of ongoing star formation. A strong bar structure appears to bisect the central bulge region. There is no visual evidence of major mergers or significant tidal disturbances, although subtle irregularities could suggest minor interactions. The dust lanes are visible along the inner edges of some spiral arms. The galaxy exhibits a moderate inclination, allowing clear observation of the spiral structure.
