This galaxy exhibits a distinct, elongated morphology, appearing cigar-shaped in its overall form. The central region presents a yellowish hue, potentially indicative of an older stellar population and/or dust obscuration. A bluer, more diffuse halo surrounds this central region, suggesting the presence of younger stars and ongoing, albeit subdued, star formation within the galactic disk. The edges of the galaxy appear relatively smooth and indistinct, lacking any prominent spiral arm structure or signs of major mergers. Overall, the galaxy's shape and color gradients imply a significant degree of ellipticity with a disk component that might be relatively small in size.
