The galaxy presents as a somewhat face-on spiral, though a significant inclination is still apparent. There is a bright, concentrated central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. The disk component shows a subtle bluish tint, suggesting ongoing star formation. The spiral arms are not sharply defined but appear flocculent and somewhat patchy. There is evidence of some minor disturbances, however a merger does not seem likely at this time. The estimated size is on the order of a few kiloparsecs. Overall, the galaxy appears to be a late-type spiral with moderate star formation activity.
