The galaxy appears to be a spiral galaxy viewed at a significant inclination. It presents a flattened, elliptical shape. A prominent bulge is observed at the center, exhibiting a yellowish-white hue, suggesting an older stellar population. Faint spiral arms extend outwards from the central bulge, displaying a bluer color, indicative of ongoing star formation. The arms appear somewhat diffuse, with a clumpy texture possibly indicating the presence of HII regions. The overall morphology leans towards a relatively smooth structure, with only subtle disturbances or irregularities. There is no obvious sign of an active galactic nucleus.
