The galaxy presents as a relatively smooth, elongated object. It exhibits a cigar-shaped morphology, with a high aspect ratio. The central region is characterized by a yellowish hue, suggesting an older stellar population, potentially indicating a concentration of evolved stars. Fainter, diffuse extensions, appearing bluish, are observed at the extremities of the galaxy along its major axis, which may indicate regions of ongoing star formation. No clear spiral arm structure or distinct dust lanes are visible in this image. Overall, the galaxy's structure seems relatively undisturbed, lacking any obvious signs of tidal interactions or major mergers.
