The galaxy presents as a cigar-shaped, relatively smooth object with a slight central bulge. The core exhibits a yellow-orange hue, possibly indicating an older stellar population or dust obscuration, while the outer edges of the disk show a bluer tint, suggesting some ongoing star formation. There is no strong evidence of spiral arm structure or a prominent bar. Minor irregularities on the periphery might point to past interactions or minor disturbances. Overall, the galaxy appears to be an elliptical or lenticular type with some residual star formation.
