The galaxy presents as a lenticular or early-type spiral, viewed at a moderately high inclination. A central bulge is visible, exhibiting a bright, concentrated luminosity. The disk component is more diffuse, with a bluer hue, possibly indicating the presence of some ongoing star formation. The morphology appears relatively undisturbed; there is no obvious evidence of recent major mergers or tidal interactions. Overall, the galaxy appears relatively smooth in texture. The disk component is elongated, giving the galaxy an overall cigar-like shape.
