The galaxy presents as a moderately inclined spiral. Two distinct spiral arms are visible, exhibiting a loose winding pattern as they emanate from the central bulge. The bulge appears moderate in size, displaying a yellowish-orange hue, indicative of an older stellar population. The spiral arms showcase a bluer tint, suggesting ongoing star formation. The overall structure exhibits slight disturbances, possibly indicating a minor interaction or past merger event. A subtle bar structure is suspected within the central region, further investigation may be required to accurately characterize the exact morphology.
