The galaxy exhibits a mostly smooth morphology, appearing as a flattened, cigar-shaped structure. The central region appears brighter and possesses a yellowish hue, which may indicate a population of older stars. Extending outwards from the center, the galaxy displays a more diffuse, bluish component. Although the galaxy shows a smooth structure, the color gradient suggests potential variations in stellar populations and star formation activity across its extent. No prominent spiral arms or strong dust lanes are discernible in this image. There appears to be no evidence of any major mergers or significant tidal disturbances affecting its structure.
