The galaxy presents a flattened, elliptical morphology, likely a disk galaxy viewed at an oblique angle. A bulge component is clearly visible, exhibiting a concentrated, yellowish hue, suggestive of an older stellar population. The disk shows evidence of spiral arm structure, though it is somewhat subdued. The arms appear tightly wound, displaying a bluer color, indicative of ongoing star formation activity. Some irregularities are present, suggesting the possibility of minor gravitational interactions or internal disturbances. The galaxy exhibits a moderate level of star formation, and a substantial stellar mass.
