The galaxy presents as a spiral type, observed at a near face-on orientation. Two distinct spiral arms emerge from the central bulge and extend outwards, displaying a loose winding pattern. The arms are traced by what appears to be active star-forming regions, indicated by a bluer hue. Dust lanes are apparent along the inner edges of the spiral arms. The central bulge exhibits a moderately bright and smooth appearance. The overall morphology suggests a galaxy that is relatively undisturbed, without significant signs of ongoing mergers or major tidal interactions, though some minor disturbances cannot be ruled out. The color profile indicates some ongoing star formation, but it does not appear to be a starburst galaxy. A weak bar might be present across the central region.
