The galaxy presents as a spiral type, with a noticeable central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter spiral arms extend outwards, appearing somewhat tightly wound. These arms are not sharply defined, but rather have a diffuse, flocculent appearance. A bluer tint is seen in some regions of the arms, indicative of ongoing star formation. The disk appears to have a moderate inclination with no visible tidal disturbances or evidence of a major merger event. There is no clear presence of a strong bar structure, but a weak central bar might be present. The galaxy is not edge-on.
