This galaxy appears to be a relatively smooth system with a slight elongation, presenting a cigar-shaped morphology. The central region exhibits a concentrated, reddish hue suggesting an older stellar population or dust obscuration. Surrounding the core, a more diffuse, bluish-green halo is visible, potentially indicative of younger star formation or a more mixed stellar population. There is little evidence of strong spiral arm structure or major disturbances, but some subtle irregularities hint at possible minor interactions or internal dynamics within the galaxy.
